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High Resolution Experimental Studies and Numerical Analysis of Fine Bubble Ozone Disinfection Contactors A Thesis Submitted to the Faculty of Drexel University by Timothy A. Bartrand in partial fulfillment of the requirements for the degree of Doctor of Philosophy Nove
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Page 1: High resolution experimental studies and numerical ...

High Resolution Experimental Studies and Numerical Analysis of Fine Bubble

Ozone Disinfection Contactors

A Thesis

Submitted to the Faculty

of

Drexel University

by

Timothy A. Bartrand

in partial fulfillment of the

requirements for the degree

of

Doctor of Philosophy

Nove

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ii

Dedications

This dissertation is dedicated to my wife, Carolyn Davis, and my daughter, Olivia

Bartrand. Few people in my station in life have the opportunity to devote time and effort

to a dissertation. That is because they don’t have a wife and daughter like mine. Thank

you both for the support, the fun, the trips to the lab and office, the loan of parts of the

house to act as my office and, above all, the love you’ve given during this process. May I

do the same for you both.

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Ackowledgements

During my dissertation studies, my work was funded by the L.D. Betz

Endowment for Environmental Engineering, the Koerner Family Fellowship, the

Philadelphia Water Department, the Steven Geigerich Schoarship, and the Northeast

Chemical Association. I am deeply grateful for the support of these organizations.

I received technical support from many during the execution of my work.

Without the help of the individuals I mention below, this work would surely have

faltered. My greatest thanks are due to my advisors, Professor Charles Haas and

Professor Bakhtier Farouk. Their assistance to me went beyond technical assistance.

They showed me, through example and in discussions, what research should and could

be. They also shared their knowledge of proposal writing and project development with

me. If, in the future, I should succeed at these endeavors it will be by following their

examples. I am grateful for the oversight and improvements in my dissertation provided

by my other committee members, Prof. Raj Mutharasan, Prof. Wen Shieh and Dr. Jin

Wen.

Others who helped me in my research at Drexel are Blaise Tobia (College of

Media, Arts and Design), who helped develop the lighting scheme I used in experiments,

Gary Burlingame, Philadelphia Water Department, who always opened his door to me

when I called, Nicole Charlton, Philadelphia Water Department, who provided a tour and

data of the Philadelphia Water Department’s pilot reactors, Dr. Patrick Gurian, for

assistance with statistics, Dr. Guibo Xie, for assistance with chemistry, and, last but not

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least, Professor Joseph Martin, for helping me find a perfect bubble column

reactor and for good conversations about engineering and beyond.

Kim DiGiovanni, Russell Goodman, Dr. Domenico Santoro, Joanna Pope, Mark

Weir, Arun Kumar and Shamia Hoque all helped in experimental data acquisition.

Thanks to them for their efforts and the cheerful way in which they offered them.

The Civil, Architectural and Environmental staff, Barbara Interlandi, Sharon

Stokes, Ken Holmes and Amanda Gonzales, are to be commended for their willingness to

help students and the collegial way they worked with them.

Finally, I acknowledge the help and camaraderie of my fellow graduate students

not yet mentioned, Dr. Dennis Greene, Dr. Bariş Kaymak, Dr. Lijie Li, Jason Marie, Dr.

Rob Ryan and Jade Blackwell. These students and those mentioned above made my

graduate studies richer and more enjoyable than I could have expected.

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Table of Contents

LIST OF TABLES..........................................................................................................VIII

LIST OF FIGURES .......................................................................................................... IX

ABSTRACT .............................................................................................................XII

I INTRODUCTION..................................................................................................... 1

I.1 Objectives and Study Overview.................................................................... 7

I.1.1 Objectives ............................................................................................ 8

I.1.2 Overview9

I.2 When and Why Ozone is Used in Water Treatment ................................... 10

I.2.1 Ozone Use in Potable Water Disinfection ......................................... 10

I.2.2 Advantages and Disadvantages of Ozone as a Disinfectant .............. 11

I.3 Ozone Contactor Design ............................................................................. 12

I.3.1 Typical Reactor Designs and Design Parameters .............................. 12

I.3.2 Reactor Design and Scale-up............................................................. 14

I.3.3 Ct Credit16

I.3.4 Roles for CFD within the Regulatory Framework ............................ 25

I.4 CFD in Water and Wastewater Treatment Operations Analysis................. 26

I.5 Need for the Current Study ......................................................................... 28

I.6 Significance of the Proposed Work............................................................. 30

I.6.1 Advancement of Knowledge ............................................................. 30

I.6.2 Value to Industry ............................................................................... 32

II LITERATURE SURVEY ....................................................................................... 35

II.1 Bubble Column Reactor Phenomena .......................................................... 37

II.1.1 Countercurrent Two-phase Flow Modeling....................................... 38

II.1.2 Ozone Demand, Decomposition and Properties................................ 83

II.1.3 Disinfection Byproduct Formation .................................................... 85

II.1.4 Microbial inactivation........................................................................ 90

II.2 Experimental Investigations of Bubble Column Reactors .......................... 94

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II.2.1 Experimental Measurement of Mass Transfer in Bubble

Columns ........................................................................................... 95

II.2.2 High-Resolution Study of Bubble Column Hydrodynamics ............. 97

II.3 Ozone Contactor Modeling ......................................................................... 99

II.3.1 CFD Models....................................................................................... 99

II.3.2 Other Models ................................................................................... 109

II.4 Other Bubble Contactor CFD Studies ....................................................... 111

III EXPERIMENTAL METHODS............................................................................ 119

III.1 Experimental Apparatus ............................................................................ 120

III.2 Residence Time Distribution Studies........................................................ 125

III.3 Ozone Mass Transfer Visualization Studies ............................................. 130

III.3.1 Overview ......................................................................................... 130

III.3.2 Indigo Dye Solution Composition and Preparation......................... 132

III.3.3 Photography Methodology .............................................................. 135

III.3.4 Development of Indigo Dye Color Calibration Curve .................... 136

IV NUMERICAL METHODS................................................................................... 143

IV.1 Mathematical Model ................................................................................. 143

IV.2 Numerical Model....................................................................................... 148

IV.3 Model Validation....................................................................................... 151

V COUNTERCURRENT FLOW HYDRODYNAMICS INVESTIGATIONS ...... 154

V.1 Bubble Plume Behavior and Flow Visualization ...................................... 155

V.2 Residence Time Distribution Analysis...................................................... 158

V.3 Numerical Studies ..................................................................................... 164

V.4 Influences of Inlet and Discharge Configurations..................................... 171

V.4.1 Philadelphia Water Department Pilot Disinfection Unit ................. 173

VI MASS TRANSFER STUDIES ............................................................................. 178

VI.1 Matrix of Mass Transfer Studies ............................................................... 178

VI.2 Ozone Mass Transfer Visualization Results ............................................. 180

VI.2.1 Observations .................................................................................... 180

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VI.2.2 Parameter Estimates......................................................................... 185

VI.3 CFD Mass Transfer Modeling Results...................................................... 209

VII CRYPTOSPORIDIUM INACTIVATION AND BROMATE FORMATION IN A

FULL-SCALE REACTOR ................................................................................... 224

VII.1 Description of Full Scale Reactor ............................................................. 224

VII.2 Full Scale Reactor CFD Model ................................................................. 226

VII.2.1CFD Model General Features .......................................................... 226

VII.2.2Cryptosporidium Inactivation and Bromate Formation Submodels 228

VII.3 Phase Distribution and Flow Field ............................................................ 229

VII.4 Inactivation and Comparison to Log Credits from Ct Models.................. 237

VIII CONCLUSIONS AND DISCUSSIONS .............................................................. 243

VIII.1 Summary of Major Findings ..................................................................... 243

VIII.2 Details of Major Findings ......................................................................... 243

VIII.3 Using CFD in Design and Scale-up of Ozone Bubble Contactors............ 249

VIII.4 Critical Review of Ozone Mass Transfer Visualization Technique.......... 252

VIII.5 Balancing Acute and Chronic Risks.......................................................... 255

LIST OF REFERENCES................................................................................................ 257

APPENDIX A:LIST OF SYMBOLS ............................................................................. 271

APPENDIX B:LIST OF ABBREVIATIONS AND ACRONYMS............................... 273

APPENDIX C:ANALYSIS OF RADIALLY-AVERAGED IMAGE DATA ............... 274

APPENDIX D:R SCRIPT FOR BEST FIT PARAMETERS ESTIMATION ............... 290

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LIST OF TABLES

Table 1: Ct Values for Cryptosporidium Inactivation by Ozone (40 CFR 141.730)......... 5

Table 2: Summary of Disinfection Impacts (United States Environmental ProtectionAgency 1999) ...................................................................................................... 6

Table 3: Advantages and Disadvantages of Ozone as a Disinfectant .............................. 12

Table 4: Guidelines for Selection of Ct Calculation Method .......................................... 17

Table 5: Summary of Bubble Diameter Relations........................................................... 47

Table 6: Summary of Gas Phase Holdup Relations......................................................... 49

Table 7: Dimensionless Parameters Associated with Bubble Drag and Terminal RiseSpeed ................................................................................................................. 51

Table 8: Summary of Bubble Drag Relations.................................................................. 54

Table 9: Summary of Bubble Terminal Speed Relations ................................................ 56

Table 10: Axial Dispersion Relations .............................................................................. 64

Table 11: Dimensionless Parameters Relevant to Bubble Column Mass Transfer ......... 67

Table 12: Summary of Mass Transfer Relations for Dispersed Bubbles in ContinuousLiquids............................................................................................................... 77

Table 13: Ozone Decomposition Rate Constants ............................................................ 84

Table 14: Factors Influencing Bromate Formation........................................................... 90

Table 15: Commonly-used Disinfection Models............................................................. 92

Table 16: Summary of Ozone Inactivation Data (Clark and Boutin 2001) ..................... 93

Table 17: Summary of Ozone Contactor CFD Studies.................................................. 108

Table 18: Comparison of Eulerian-Eulerian and Eulerian-Lagrangian Approaches ..... 117

Table 19: Countercurrent Flow Hydrodynamics Experimental and Numerical Studies 154

Table 20: Countercurrent Flow Peclet Number Relations............................................. 161

Table 21: Mass Transfer Visualization Experiments..................................................... 179

Table 22: Best Fit Parameters ........................................................................................ 204

Table 23: Rate Expressions and Constants, Full Scale CFD Model.............................. 229

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LIST OF FIGURES

Figure 1: Inactivation and DBP Formation for a Hypothetical Water............................... 3

Figure 2: Schematic Diagram of a Full Scale Ozone Bubble Contactor ......................... 13

Figure 3: Segregated Flow Analysis Illustration ............................................................. 21

Figure 4: Extended CSTR Method Illustration................................................................ 23

Figure 5: Interrelated Processes in a Bubble Column (adapted from Heijnen and Van'tRiet (1984)) ....................................................................................................... 38

Figure 6: Illustration of Homogeneous and Heterogeneous Bubbly Flow (Camarasa etal., 1999)............................................................................................................ 39

Figure 7: Countercurrent Bubble Column Flow Regimes Schematic Diagram (adapatedfrom Uchida, Tsuyutani et al. (1989) ................................................................ 41

Figure 8: Bubble Rise Velocity and Discharge Coefficient Schematics (Moore 1959) .. 53

Figure 9: Migration of a Bubble Plume to a Wall (Freire et al., 2002) ........................... 59

Figure 10: Migration of Bubble Plumes toward Each Other (Freire et al., 2002) ........... 60

Figure 11: Schematic Diagram of the Two-Film Mass Transfer Model ......................... 68

Figure 12: The Hydrodynamics of the Transport of Ozone from Gas Phase to the BulkLiquid Phase ...................................................................................................... 71

Figure 13: Significant Ozone Disinfection Byproducts (Song et al., 1997; United StatesEnvironmental Protection Agency 1999; von Gunten 2003b) .......................... 86

Figure 14: Bromate Formation Pathways (Song et al., 1997).......................................... 88

Figure 15: Ozone Contactor Design Modifications (Henry and Freeman 1995)........... 101

Figure 16: Murrer, Gunstead et al. (1995) Reactor Schematic ...................................... 103

Figure 17: Reactor Schematic for Cockx CFD Study.................................................... 105

Figure 18: Experimental Reactor Photograph................................................................ 121

Figure 19: Laboratory Bubble Column Schematic Diagram (not to scale) ................... 123

Figure 20: Reactor Schematic Diagram, Scale Drawing ............................................... 124

Figure 21: Scale Drawing of Laboratory Column Bottom ............................................ 124

Figure 22: Conductivity Probe Calibration.................................................................... 126

Figure 23: Typical Tracer Curve.................................................................................... 127

Figure 24: RTD Model Schematic Diagrams ................................................................ 128

Figure 25: Indigo Trisulfonate Structure and Daughter Products.................................. 134

Figure 26: Mass Transfer Visualization Experiment Lighting ...................................... 136

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Figure 27: Pixel Color Calibration Images .................................................................... 138

Figure 28: Calibration Image Histograms...................................................................... 139

Figure 29: Variation of Absorbance with Indigo Concentration for Indigo ReagentDiluted with Tap Water................................................................................... 140

Figure 30: Pixel Color Calibration Curve...................................................................... 142

Figure 31: Diameter Along which Grid Resolution Study was Performed ................... 150

Figure 32: Gas Volume Fraction Profiles ...................................................................... 151

Figure 33: CFD Model Validation................................................................................. 153

Figure 34: Photographs of Bubble Plume Shapes.......................................................... 155

Figure 35: Flow Visualization – Dye Progress at 30s, 1 min, 1 min 30s and 2 min (theDark Triangle Approximately 1/3 the Reactor Height in Each Image is theGlass Maker’s Manufacturer’s Mark) ............................................................. 157

Figure 36: Experimental Residence Time Distributions (RTDs) for 0 < Qg < 3 L/min 159

Figure 37: Experimental and Predicted Peclet Number................................................. 162

Figure 38: Virtual Tracer Concentration at 20s, 40s and 60s after Step Input .............. 165

Figure 39: Phase Distribution ........................................................................................ 167

Figure 40: Water Velocity Vectors near the Diffuser.................................................... 168

Figure 41: Spatial Variations in Mixing ........................................................................ 170

Figure 42: Typical Intake Configuration for Countercurrent Full Scale Ozonation...... 172

Figure 43: Philadelphia Water Department Pilot Column Phase Distribution .............. 175

Figure 44: PWD Pilot Reactor Intake and Discharge Region Velocity Vectors ........... 176

Figure 45: PWD Virtual Tracer Study ........................................................................... 177

Figure 46: Indigo Dye Decoloration Images ................................................................. 181

Figure 47: Eddy Transport during Ozonation................................................................ 184

Figure 48: Illustration of Well-Mixed Zone and Radially-Averaged Concentration .... 186

Figure 49: Identification of Best Fit Critical Depth....................................................... 192

Figure 50: Mass Transfer Visualization, Qgas = 0.4 slpm, QL = 7.0 lpm, Case A ......... 195

Figure 60: Variation of Entrance Region Length with Gas to Liquid Flow Ratio ........ 206

Figure 61: Variation of Zone 1 Stanton Number with Gas to Liquid Flow Ratio ......... 207

Figure 62: Variation of Zone 1 Peclet Number with Gas to Liquid Flow Ratio ........... 208

Figure 63: Sample Locations ......................................................................................... 211

Figure 64: Predicted and Measured Indigo Dye Concentrations ................................... 212

Figure 65: Image Location, Experimental Images and CFD ......................................... 213

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Figure 70: Comparison of CFD and Experimental Indigo Dye ConcentrationData, Q6=0.4 slpm, QL=7.0 lpm ...................................................................... 220

Figure 71: Comparison of CFD and Experimental Indigo Dye Concentration Data,Q6=0.4 slpm, QL=13.5 lpm.............................................................................. 221

Figure 72: Comparison of CFD and Experimental Indigo Dye Concentration Data,Q6=0.7 slpm, QL=7.0 lpm................................................................................ 222

Figure 73: Comparison of CFD and Experimental Indigo Dye Concentration Data,Q6=0.7 slpm, QL13.5 lpm ................................................................................ 223

Figure 74: ACWD Full Scale Reactor Schematic Diagram........................................... 226

Figure 75: Full Scale Reactor CFD Model Schematic Diagram.................................... 227

Figure 76: Gas Volume Fraction Contours, Full Scale Reactor, Vertical Plane............ 230

Figure 77: Gas Volume Fraction Contours, Full Scale Reactor, Horizontal Plane near theSpargers ........................................................................................................... 231

Figure 78: Gas Volume Fraction Contours, Full Scale Reactor, Horizontal Plane at theReactor Mid-height ......................................................................................... 232

Figure 79: Water Superficial Velocity Vectors, Chambers 1 - 5, Full Scale Reactor ... 234

Figure 80: Water Superficial Velocity Vectors, Chambers 6 - 10, Full Scale Reactor . 235

Figure 81: Water Superficial Velocity Vectors, Full Scale Reactor, Horizontal Plane,Chambers 1 – 4, Projection Tangential to Plane ............................................. 236

Figure 82: Water Superficial Velocity Vectors, Full Scale Reactor, Horizontal Plane,Chambers 5 – 10, Projection Tangential to Plane ........................................... 237

Figure 83: Dissolved Ozone Concentration Contours, Full Scale Reactor.................... 238

Figure 84: Bromate Concentration Contours, Full Scale Reactor ................................. 240

Figure 85: Cryptosporidium parvum Density Contours, Full Scale Reactor................. 242

Figure 86: Alternate Lighting Scheme........................................................................... 254

Figure 87: Conservation of Gas Phase Ozone and Aqueous Indigo Dye ...................... 275

Figure 88: Schematic Diagram, Two-Zone Model ........................................................ 283

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ABSTRACT

Countercurrent flow hydrodynamics and mass transfer were explored using

computational fluid dynamics (CFD) analyses, tracer studies and a novel mass transfer

visualization technique. In concert, these techniques yielded a comprehensive description

of countercurrent hydrodynamics and mass transfer.

In the laboratory bubble column reactor in which experimental studies were

performed, liquid flowed upward with gas bubbles in the core of the bubble plume and

downward outside the bubble plume near the cylinder walls at all gas flow rates. CFD

predicted a large recirculating flow near the sparger. Well-mixed conditions were

observed in a zone termed the entrance length, located near the sparger. Mass transfer

visualization experiments allowed estimation of the entrance region length. The entrance

region increased as a function of gas flow rate and ranged from a value of about 22% (for

the lowest gas to liquid flow ratio experiment) to nearly 40% (for the highest gas to liquid

flow ratio experiment.

To demonstrate its utility as a design tool or for troubleshooting underperforming

full scale reactors, CFD was used to predict hydrodynamics, Cryptosporidium parvum

inactivation and bromate formation in a full scale reactor. Despite being relatively crude

the CFD model identified flowfield features conducive to bromate formation or

deleterious to C. parvum inactivation. Specifically, in chambers in which ozone is

applied, large recirculating flows were predicted. Water detained in these recirculating

flows have relatively long detention times and contribute to bromate formation in waters

with sufficient bromide content.

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The current study demonstrates that, even in a simple tall right circular

cylindrical bubble column, hydrodynamics plays a major role in contact of ozone with

microorganisms and substances that form bromate. Both experimental and analytical

studies identified significant spatial variations in mixing and mass transfer in the

relatively simple bubble column reactor. These findings indicate that CFD could be more

widely used as a component of pilot scale studies of ozone bubble contactor reactors or in

design of full scale contactors. Given current computer prices and speeds, CFD analysis

is appropriate for plants with capacities which are smaller than the very large capacity

plants for which CFD is presently used.

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I INTRODUCTION

Thorough, efficient water disinfection requires sustained, uniform contact

between pathogenic organisms suspended in the water and dissolved disinfectant. The

most frequent way of assessing the extent of disinfectant-pathogen contact is through

estimation of “Ct,” where C is the disinfectant residual and t is the contact time between

disinfectant and organisms.

The disinfectant residual is seldom uniform or steady. Chemical disinfectants

react and decay. Mixing of disinfectant with pathogen-laden water may be incomplete.

In ultraviolet disinfection processes, shielding or variations in distance between

pathogens and the UV source may result in non-uniform contact between disinfectant and

microorganisms. To account for spatial and temporal variations in disinfectant-organism

contact and disinfectant residual, estimates for “Ct” are made using conservative

estimates for contact time and disinfectant concentration, such as the time required for

10% of a conservative tracer to exit the reactor in a pulse tracer experiment (T10) and the

disinfectant residual at the reactor discharge or discharge from individual chambers in the

reactor (Lev and Regli 1992a; Lev and Regli 1992b).

Beyond having to account for uneven contact between organisms and disinfectant,

regulatory agencies must also apply safety factors to estimated Ct values to account for

uncertainty in inactivation rate models and for the influence of water matrix constituents

and varying water quality properties on inactivation rate. For example, given the wide

variation in observed Cryptosporidium parvum inactivation rates, disinfection goals up to

1 log-unit higher than desired disinfection goals may be required to ensure actual

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inactivation is within 95% confidence bounds of predicted inactivation (Finch et

al., 2001).

There are drawbacks to the protective design approach to disinfection process

design criteria described above – disinfection byproduct (DBP) formation and excessive

energy consumption and chemical dosing. Depending on the composition of the water

that is disinfected and the disinfectant used, byproducts that pose chronic human health

risks may be formed during disinfection. Chlorine-based disinfectants produce

trihalomethanes (THMs) and haloacetic acids (HAAs) among other byproducts. THMs

and HAAs are regulated under the Disinfectant and Disinfectant Byproducts rule (US

EPA Office of Water 2001) and numerous community public water treatment facilities

have been out of compliance with these regulations since their promulgation (US EPA

2005).

As will be described in Chapter 2, ozone produces fewer and lower concentrations

of DBPs than chlorine, except in waters high in bromide (Br -). In those waters,

depending on the pH, ammonia concentration, temperature, alkalinity and dissolved

organic carbon concentration, bromate (BrO3-), a suspected human carcinogen, may be

formed. The US EPA’s current maximum contaminant level (MCL) for bromate is 10

g/L.

Microbial inactivation and DBP formation processes occur at the same time scale,

as illustrated in Figure 1. Taking Ct to indicate a level of disinfection, the plot shows

exposure to Cryptosporidium parvum oocysts and bromate commensurate with a range of

disinfection levels. The dashed curve showing reduction in Cryptosporidium parvum is

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based on an inactivation rate model derived from batch studies of

Cryptosporidium inactivated in filtered water (Finch et al., 2001). The bromate

formation curve was developed based on regression analysis of bromate formation rate

data and is drawn for filtered water with a relatively high (170 g/L) initial bromide ion

concentration (Song et al., 1996). Recalling that the current MCL for bromate is 10 g/L,

achieving a design reduction in Cryptosporidium parvum of 2 logs using only ozone

disinfection is not possible without exceeding the bromate MCL unless steps are taken to

enhance inactivation or retard bromate formation. If appropriate safety factors protective

of microbiological quality are employed, bromate concentration will exceed the MCL by

an even greater amount.

Figure 1: Inactivation and DBP Formation for a Hypothetical Water

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In chlorine-based disinfection, chemical disinfectant is introduced to the

treatment train as a solution and is mixed with process water prior to introduction to the

disinfection processes. After the disinfectant demand of the raw water is satisfied, the rate

of decay of active forms of chlorine is slow relative to typical retention times in

disinfection processes and the chlorine concentration does not vary significantly in the

reactor. In ozone disinfection, water enters the reactor with no ozone and ozone is

dissolved into process water in early stages of the disinfection process. There is often

significant ozone demand in the early portion of an ozonation process. For example, in a

pilot study of ozonation of Central Arizona Project (CAP) water, identical ozone doses

were applied to two identical cylindrical contactors arranged in series and operating in

countercurrent mode. When the contact time in the cylinders was large (above 7.5

minutes) the increase in ozone residual between the intake and discharge in the second

column was double that of the first column (Nieminski 1990). The rate of decay of ozone

is also significantly higher than that of chlorine disinfectants, especially for water at

temperatures above 20°C or that are slightly basic (Rakness 2005). Thus, ozone

concentration varies more widely than that of chlorine in disinfection processes.

Because the number of pathogens present in treated drinking water is very low,

regulating disinfection processes based on detection of pathogens in reasonably sized

samples is not possible. Rather, the United States Environmental Protection Agency

grants “disinfection credits” for well-operated filtration processes, disinfection and, in

recent amendments to the safe drinking water act, demonstration of high source water

quality and protection (42 U.S.C. 300g-1(b)(7)(C)(iv)). Plants receive “Ct credit” based

on measured or estimated hydraulic characteristics of unit process operations and based

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on batch kinetic studies of their disinfectant’s decay rate in the plant’s water. Ct

credit for disinfection processes is established based on measurement of disinfectant dose

at the reactor discharge and intermediate locations and on either measured residence time

distributions (RTDs) or using hydraulic models such as continuously stirred tank reactors

(CSTRs) for assessing reactor hydraulics. The Ct required to achieve a desired reduction

in microbial concentration depends on the disinfectant, the microorganism, water

properties (primarily pH and temperature) and constituents, initial microbial density, and

possibly other factors. Log credit awarded by EPA for Cryptosporidium inactivation by

ozone is presented in Table 1.

Table 1: Ct Values for Cryptosporidium Inactivation by Ozone (40 CFR 141.730)

Water Temperature (ºC)Logcredit 0.5 1 2 3 5 7 10 15 20 25

0.5 12 12 10 9.5 7.9 6.5 4.9 3.1 2.0 1.2

1.0 24 23 21 19 16 13 9.6 6.2 3.9 2.5

1.5 36 35 31 29 24 20 15 9.3 5.9 3.7

2.0 48 46 42 38 32 26 20 12 7.8 4.9

2.5 60 58 52 48 40 33 25 16 9.8 6.2

3.0 72 69 63 57 47 39 30 19 12 7.4

The current conservative approach to disinfection is evident in the assessment and

assignment of treatment plant Ct described above. Table 2 provides an overview of the

disinfection/byproduct tradeoff. Source waters carry with them varying loads of

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pathogenic organisms and chemical compounds and have diverse physical

properties. Given these complexities, establishing an optimal reactor design that provides

sufficient disinfection and minimizes disinfection byproduct formation is clearly a

formidable task that will require significant experimental studies and modeling.

Table 2: Summary of Disinfection Impacts (United States EnvironmentalProtection Agency 1999)

Disinfection parameter Typical impact on pathogeninactivation

Typical impact on DBP formation

Disinfectant type Depends on inactivation efficacy Depends on disinfectant reactivity

Disinfectant strength The stronger the disinfectant, thefaster the disinfection process.

The stronger the disinfectant, thegreater the production of DBPs.

Disinfectant dose Increasing the disinfectant doseincreases the disinfection rate

Increasing the disinfectant dosetypically increases the rate of DBPformation

Type of organism Susceptibility to disinfection variesaccording to pathogen group. Ingeneral, protozoa are more resistantto disinfectants than bacteria andviruses.

None.

Contact time Increasing the contact timedecreases the disinfectant doserequired for a given level ofinactivation

Increasing the contact time with anequivalent disinfectant dose increasesthe formation of DBPs.

pH pH may affect the disinfectant formand, in-turn, the efficiency of thedisinfectant.

The impact of pH varies with DBP.For ozonated water containing bromideion, high pH favors the formation ofbromate ion and low pH favorsformation of brominated organicbyproducts.

Temperature Increasing temperature increasesthe rate of disinfection.

Increasing temperature typicallypromotes faster oxidation kinetics and,hence, increases DBP formation.

Turbidity Particles responsible for turbiditycan surround and shield pathogenicmicroorganisms from disinfectants.

Increased turbidity may be associatedwith increased NOM, which representsan increased amount of DBPprecursors for the formation of DBPswhen disinfectant is applied.

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Disinfection parameter Typical impact on pathogeninactivation

Typical impact on DBP formation

Dissolved organics Dissolved organics can interferewith disinfection by creatingdemand and reducing the amountof disinfectant available forpathogen inactivation.

Increased dissolved organics willrepresent a larger amount of DBPprecursor for the formation of DBPswhen the disinfectant is applied.

I.1 Objectives and Study Overview

The current study provides detailed quantitative information on the mixing and

mass transfer processes for dissolution of ozone in countercurrent flow and demonstrates

use of a detailed model for design and analysis of ozone bubble contactors. These

detailed measurements and analyses are intended to allow more precise prediction of

ozone mass transfer, microbial disinfection and chemical byproduct formation and can be

used to strike a balance allowing management of acute risk of microbial infection and

management of chronic risks associated with disinfection byproducts.

As described in the following chapter, many mass transfer relations for

dissolution of gases from bubbles have uncertain applicability at conditions differing

from those in which the data from which they were developed were collected.

Specifically, many relations found in the literature were developed for co-current bubble

contactors or are theoretical relations developed without concern over the interactions

between the liquid flow field and bubble plume and their impacts on mass transfer. None

of the mass transfer studies described in the literature review included an assessment of

axial variations in mass transfer. Mass transfer studies and mass transfer relations drawn

from the literature are described in detail in section II.1.1.5. Given the marked difference

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in the distribution of bubbles and their momentum near the sparger compared

with their distribution and momentum away from the sparger, these axial variations are

expected to be significant and should be explored.

I.1.1 Objectives

The goal of the present work was to quantify the influence of non-ideal

hydrodynamics on mass transfer and contact of dissolved ozone with pathogens in

countercurrent bubbly flow. The objectives of this work were to:

Quantify dispersion (inclusive of axial variations) in a laboratory countercurrent flow

bubble column reactor using experimental residence time distribution studies and

computational fluid dynamic (CFD) modeling and relate the dispersion to reactor

operating conditions and geometry;

Use a novel visualization technique for observing ozone mass transfer (inclusive of

axial variations) in the bubble column and determine whether axial variations in mass

transfer significantly impact the ability of engineers to scale up countercurrent flow

reactors;

Validate a CFD model for ozone mass transfer in countercurrent flow and assess the

accuracy of the mass transfer model in predicting mass transfer in countercurrent

flow; and

Demonstrate the ability of the validated CFD model to simultaneously predict

Cryptosporidium parvum inactivation and bromate formation in a full-scale reactor

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9

and identify advantages and disadvantages of CFD compared with design

models currently used in ozone bubble contactor design and Ct credit assessments.

I.1.2 Overview

To achieve these objectives, two sets of experiments were performed and a CFD

model of countercurrent ozone mass transfer, inclusive of relevant chemistry and

microbial inactivation, was developed and exercised. The two sets of laboratory

experiments were

tracer studies performed to quantify mixing and hydrodynamics in countercurrent

gas-liquid flow and

ozone mass transfer visualization studies performed to enable estimation of mass

transfer rate and identify spatial variations in mass transfer.

The CFD model was developed using the commercial CFD code CFX (ANSYS

Inc. 2004) and was validated using data taken in both the tracer studies and mass transfer

visualization studies. Results from CFD studies were compared with those of

experimental studies, providing explanation for trends observed. Finally, a CFD model

was developed and executed for simultaneous prediction of Cryptosporidium parvum

inactivation and bromate formation in a full scale reactor.

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10

I.2 When and Why Ozone is Used in Water Treatment

I.2.1 Ozone Use in Potable Water Disinfection

In general, potable water1 disinfectants are strong oxidants and may serve

multiple purposes in the water treatment process. These may include (United States

Environmental Protection Agency 1999):

Inactivation of pathogenic organisms;

Control of aquatic nuisance species;

Oxidation of iron and manganese;

Removal of compounds causing tastes and odors;

Improvement of coagulation (and subsequent filtration);

Removal of color;

Prevention of algal growth in sedimentation basins and filters; and

Prevention of biological regrowth in distribution systems.

Thus, selection of a chemical for water disinfection may be guided by its use in other

processes in water treatment as well as its ability to kill pathogenic organisms.

Chlorine remains the most widely used disinfectant in the United States. As of

2000, The United States Environmental Protection Agency reports that 68.7% of

1 In the remainder of this thesis, all processes will be assumed to be for potable water treatment

and the modifier “potable water” will be omitted.

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11

community water systems (systems providing service connections and year-

round service to at least 15 connections or 25 people, inclusive of those required to

disinfect and those exempt) use chlorine downstream of filtration (for those plants

employing filtration) (United States Environmental Protection Agency 2000). This

percentage includes plants using one or more disinfectants in conjunction with chlorine.

Only 0.4% of plants report using ozone downstream of filtration, though 3.5% of

reporting plants use ozone for predisinfection or oxidation upstream of filtration.

However, as American utilities strive to meet disinfection and disinfection

byproduct goals required by the Stage 1 Disinfectants and Disinfection Byproducts Rule

and Long Term 2 Enhanced Surface Water Treatment Rule (LT2SWTR), plants are

assessing ozone disinfection as an alternative, particularly for Cryptosporidium parvum

inactivation and for disinfection byproduct minimization.

I.2.2 Advantages and Disadvantages of Ozone as a Disinfectant

The impetuses for recent increases in the number of U.S. water treatment plants

incorporating ozone disinfection into treatment are concerns over chlorine-resistant

organisms and disinfection byproducts. Specifically, ozone is the only chemical

disinfectant that inactivates Cryptosporidium parvum at doses and contact times

realizable in treatment plants and does not produce the halogen-substitute byproducts

typical of water treated with chlorine. The advantages and disadvantages of ozone

disinfection (compared with other schemes) are summarized in Table 3 (US EPA Office

of Water 1999).

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12

Table 3: Advantages and Disadvantages of Ozone as a Disinfectant

Advantages Disadvantages

More effective than chlorine,chlorine dioxide, chloramines forinactivation of viruses,Cryptosporidium parvum andGiardia

Efficient chemical disinfectantrequiring relatively short contacttime

In the absence of bromide, halogen-substitute DBPs are not formed.

Ozone is a strong oxidant andcontrols odor, color and taste

Produces disinfection byproductsincluding products of bromide(primarily bromate), aldehydes,ketones and others.

High capital and operating costs

Ozone is corrosive and toxic

Ozone provides no residual

Ozone decays rapidly at high pHand warm temperatures

I.3 Ozone Contactor Design

I.3.1 Typical Reactor Designs and Design Parameters

Gaddis (1999) lists potential gas-liquid contactors (excluding surface contactors

which would be inappropriate for ozonated water) as bubble columns, stirred vessels, jet

loop reactors and impinging stream reactors. Among these, the bubble column has the

lowest volumetric mass transfer coefficient but offers the advantages of simple design

and operation, high interfacial transfer area (to account for a much higher liquid film

resistance to mass transfer than gas film resistance) and, when well-designed, a greater

propensity toward plug flow hydraulics. Thus, ozone contactors are often bubble

columns. Shah, Kelkar et al. (1982) state that bubble contactors are well suited for slow

liquid phase reactions (such as microbial inactivation by dissolved ozone gas) due to high

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13

transport rates between phases, high interfacial area, large liquid holdup and the

absence of moving parts.

A schematic diagram showing typical ozone bubble contactor configuration is

found in Figure 2 (based on Cockx et al., 1999). Countercurrent and co-cocurrent flow

may be encountered, though countercurrent contact between bubbles and liquid is more

common (Rakness 2005). Industrial ozone bubble contactors are typically on the order of

4 m tall and employ baffling as shown in Figure 2 to promote uniform contact between

the phases and distribution of ozone in the untreated water. Off gas from industrial

bubble contactors is collected and either destroyed or recycled and reinjected into the

water.

Waterinlet

Outlet

Ozonated air

Waterinlet

Outlet

Ozonated air

Figure 2: Schematic Diagram of a Full Scale Ozone Bubble Contactor

The bubble contactor design features that determine contactor performance and

over which engineers have control are (Do-Quang et al., 2000):

Contactor geometry;

Gas/water flow rates:

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14

Gas/water flow ratio; and

Diffuser positions.

The choice of these design and operating parameters determines bubble contactor

performance and is manifested in gas holdup distribution, liquid phase mixing, mass

transfer coefficients, bubble size distribution and coalescence (Sanyal et al., 1999).

Geometric features of contactors demonstrated to significantly improve hydraulic

performance (increase the ratio of T10 to hydraulic residence time) are addition of baffles

(especially double baffles), use of spargers that produce fine bubbles, and uniform

distribution of spargers along the contactor bottom (Henry and Freeman 1995; Do-Quang

et al., 2000). Design features that have shown only minor influence on reactor hydraulics

performance are addition of corner fillets and wall foils.

I.3.2 Reactor Design and Scale-up

With the possible exception of CFD analyses, there are no models or fundamental

theories capable of a priori, dependable prediction of liquid phase mass transfer

coefficients or gas phase holdups for multiphase flow reactors (Nauman 2001). Factors

such as non-ideal reactor hydrodynamics, variations in liquid or gas composition and

quality, and transient operation influence mass transfer rate. So full scale ozone bubble

contactor reactor designs are based on measurements taken in bench scale semi-batch or

batch experiments performed in well-stirred reactors or on measurements in continuous

flow pilot systems.

To the extent possible, engineers are advised to design pilot and bench scale

reactors that physically resemble full scale reactors (Langlais et al., 1991), giving rise to a

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15

chicken and egg dilemma. Scale-up of semi-batch systems can be done

effectively – Rakness (2005) reports nearly identical predicted and realized performance

for a full scale ozone contactor designed based on semi-batch data. One possible

explanation for this agreement is that the chambers in the full-scale contactor perform as

continuously stirred tank reactors (CSTRs) and that the hydrodynamics closely resemble

those in semi-batch experiments. The positive side of this agreement is that the full scale

contactor achieved design goals. The negative side is that, if the chambers are behaving

as CSTRs, ozone transfer and inactivation are less than they would be if the contactor had

been designed with hydraulics closer to plug flow.

Often, in pilot studies gas phase ozone concentration is measured only at the

reactor intake and in the off-gas and ozone mass transfer is quantified via the transferred

dose or the transfer efficiency (100% transfer dose/applied dose) (Langlais et al., 1991;

Rakness 2005). Because ozone contactors are invariably designed with relatively low gas

to liquid flow ratios, transfer efficiency is almost always very high (> 95%). Commonly,

design engineers simply assume that transfer efficiency of typical bubble contactors is in

the range 90% to 95% (Schulz et al., 2003). Such gross mass transfer data and

assumptions provide no information on where in the reactor the mass transfer occurs and

provide no guidance on the optimal liquid phase depth, despite the goal of setting full

scale reactor depth to ensure high transfer efficiency and minimize ozone production

costs (Langlais et al., 1991).

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16

I.3.3 Ct Credit

As described above, utilities demonstrate compliance with water disinfection

regulations by obtaining “Ct” credits based on design and operation of bubble contactors,

not through direct measurement of reduction in microbial loads in the process stream. A

description of how Ct is calculated follows. This discussion is important because

meeting Ct requirements is the primary design goal for engineers designing ozone bubble

column reactors. For the work presented in this dissertation to be of practical use in the

water treatment industry, it must be applicable within the framework of the current

regulatory system or it must present alternative methods for ensuring adequate

disinfection.

The US EPA has approved assessment of Ct in ozone bubble contactors via one of

four prescribed models (described below) or via a site specific evaluation (US EPA

Office of Water 2003; Rakness 2005). The models allowable for claiming Ct credit in

ozone bubble contactors are:

The T10 method,

segregated flow analysis (SFA);

completely stirred tank reactor (CSTR) analysis; or

extended CSTR analysis.

Guidelines for selection of Ct calculation method from EPA’s guidance for

compliance with the Long Term 2 Enhanced Surface Water Treatment Rule

(LT2ESWTR) are presented in Table 4.

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Table 4: Guidelines for Selection of Ct Calculation Method

Sectiondescription Terminology

Method forcalculating loginactivation Restrictions

Chambers where ozone is added

First chamber First dissolutionchamber

No log inactivationcredit isrecommended

None

OtherChambers

Co-current orcounter-currentdissolutionchambers

CSTR method in eachchamber w/ ameasured effluentresidual concentration

No credit given to a dissolutionchamber unless detectable ozoneresidual is measured upstream of thechamber

Reactive Chambers

3consecutivereactivechambers

Extended CSTRzone

Extended CSTRmethod in eachchamber

Detectable ozone residual should bepresent in at least 3 chambers inzone, measured via in-situ sampleports. Otherwise, apply CSTRmethod individually to eachchamber with a measured O3

residual

No

trac

erd

ata

< 3Consecutivechambers

CSTR reactivechambers

CSTR method in eachchamber with ameasured ozoneresidual concentration

None

Chambers where ozone is added

First chamber First dissolutionchamber

No log inactivationcredit isrecommended

None

OtherChambers

Co-current orcounter-currentdissolutionchambers

T10 or CSTR methodin each chamber

No credit is given to a dissolutionchamber unless a detectable ozoneresidual is measured upstream of thechamber

Reactive chambers

3consecutivereactivechambers

Extended CSTRzone

Extended CSTRmethod in eachchamber

Detectable ozone residual should bepresent in at least 3 chambers inzone, measured via in-situ sampleports. Otherwise, apply the T10 -CSTR method individually to eachchamber with a measured O3

residual

Wit

htr

acer

dat

a

< 3Consecutivechambers

CSTR reactivechambers

CSTR method in eachchamber with ameasured ozoneresidual concentration

None

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The compliance guidance for the LT2ESWTR has been withdrawn

pending revision, though the draft guidance (US EPA Office of Water 2003) is referenced

in this dissertation. The LT2ESWTR allows calculation of Ct using the extended CSTR

method (described below) in addition to the methods allowed under the Surface Water

Treatment Rule (SWTR) (US EPA Office of Drinking Water 1991).

I.3.3.1 The T10 Method

In the T10 method, conservative estimates for the residence time of fluid elements

in the reactor and the average ozone concentration in the elements during their residence

are made and Ct is the product of the estimates. T10, the time required 10% of a

conservative tracer introduced as a pulse at the reactor inlet to exit the reactor, has been

shown to provide a conservative estimate of the time fluid elements spend in a reactor,

whether flow in the reactor approaches that in a CSTR or that of an advection-dispersion-

reaction model (Lev and Regli 1992b). Since the ozone concentration varies from

chamber to chamber in a multi-chamber reactor (such as the one depicted in Figure 2), it

is necessary to estimate the T10 for individual chambers separately. In the absence of

tracer data for individual chambers, it is assumed that the T10 of individual chambers

scales with the overall system T10 according to

system,10

system

subunitsubunit,10 T

V

VT

(1)

where subunitV is the volume of the subunit and systemV is volume of the overall system.

According to the authors, equation 1 provides a reasonable estimate of subunit T10 for

subunits whose volume is less than 50% the total reactor volume.

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19

Because ozone undergoes autodecomposition in water, ozone

concentration is not constant in contactors and the average ozone concentration in

subunits of the reactor must be estimated for use in Ct calculations. The mode of

operation (countercurrent two-phase flow, co-current two phase flow or reactive segment

[with no ozone application]) in a given reactor subunit dictates the way the average ozone

concentration is calculated. It is assumed that, because of ozone demand and decay, no

significant ozone residual is achieved in the first chamber of an ozone bubble contactor in

which ozone is applied. In subsequent chambers, the following guidelines apply (Lev

and Regli 1992a):

segmentsReactive

operationCocurrentor

32operation;rentCountercur

chamberndissolutioFirst0

out

outinout21

out

avg

C

CCC

ssCC (2)

In equation 2, Cavg is the average ozone concentration in a subunit, Cout is ozone

concentration at the subunit discharge, Cin is the ozone concentration at the subunit inlet

and s is a safety factor. When ozone decomposition rate is high, the safety factor

approaches the value 3; when decomposition rate is low, it approaches 2.

I.3.3.2 CSTR Analysis

The CSTR analysis (described below) is appropriate for

reactors whose flow approaches that of a CSTR,

reactors with only one chamber and for which T10 / HDT < 0.33 and required

inactivation level for Giardia greater than or equal to 2.5 logs, and

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20

reactors for which there are no tracer data (U.S. EPA Office of Drinking

Water 1991).

Assuming disinfectant and microorganisms are homogenously distributed within a

reactor chamber and that inactivation of microorganisms is first order with respect to

microorgansism concentration and disinfectant concentration (Chick kinetics), the Ct that

achieves a survival ratio of 0NN (concentration of surviving organisms divided by

concentration of organisms introduced to the chamber) is given by

0

0

303.2

1HDT

NNk

NNC

(3)

In equation 3, HDT is the theoretical hydraulic detention time (chamber volume

volumetric flow rate) and k is the inactivation rate constant (assuming first order kinetics

with respect to microorganism density and disinfectant concentration) for the

microorgansism of interest. At present, the two organisms believed most resistant to

disinfection are Giardia and Cryptosporidium and Ct is calculated for one or both of

those organisms. The inactivation rate constant may be determined via batch kinetic

studies (the preferable method) or drawn from tables of inactivation rate constants

published by the EPA.

I.3.3.3 Segregated Flow Analysis

In the segregated flow analysis (SFA), it is assumed that the inactivation achieved

in a reactor is proportional to two probabilities: the probability that a microorganism

remains in the reactor for a specified time and the probability that the microorganism is

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21

inactivated if exposed to disinfectant for the specified time. The segregated

flow model is illustrated in Figure 3.

12

3

4

1

2

3

4

t

Width of bars is proportional to fraction of flowthrough the segment

Figure 3: Segregated Flow Analysis Illustration

The probability distribution for water (and microorganism) residence times, E(t),

is determined via tracer studies and residence time distribution analyses (Danckwerts

1953; Haas et al., 1997). The probability of inactivation over a time period, t, is

calculated using a modified form of Chick’s law (Trussell and Chao 1977):

kCt

N

N 100

(4)

Note that in equation 4 that the ozone residual concentration, C, is assumed constant with

respect to time. The EPA’s guidance does not provide explicit instructions on the value

of ozone concentration for use in equation 4.

The overall probability of organism survival is then

n

i

Ctk

iitE

N

N

10

10 (5)

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22

where n is the number of segments into which the flow was divided. Equation

5 may be used to determine the concentration, C, required to achieve a desired level of

disinfection.

I.3.3.4 Extended CSTR Analysis

In the extended CSTR method, three or more consecutive reactive chambers

(chambers without ozone addition) can be analyzed as consecutive CSTRs (US EPA

Office of Water 2003). In the ozone bubble contactor shown in Figure 4 (based on the

example of the extended CSTR method provided by Rakness (2005)), the reaction zone

over which the extended CSTR method may be used to estimate inactivation is comprised

of all the chambers downstream of chamber 1 (in which ozone is applied). Each of the

chambers is treated as a CSTR. Three sample points, S1, S2 and S3 are shown. The

ozone residual is measured at each o those sample points and used in estimation of the

ozone decay rate and average residual in each chamber. The advantages of the extended

CSTR method are that it requires very little experimental data and that it accounts for

ozone decay more systematically than the other Ct analyses.

The ozone decay rate, k*, in the reactor is estimated based on the difference in

ozone residual measurements made at sample ports 1 and 2 and between sample ports 1

and 3. Sample location one should be at least one chamber downstream of the discharge

of a chamber in which ozone is applied. This ensures that most of the ozone demand has

been exerted and measured differences in ozone concentration are due to

autodecomposition.

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23

1 2 3 4 5 6 7 8

S1

S2 S3

Reaction zone

Reaction zone hydraulic detention time

Ozo

nere

sid

ual

(mg

/L)

Figure 4: Extended CSTR Method Illustration

Assuming all chambers are CSTRs, the decay rate between sample locations i and

j is given by

1HDT

1

*

jin

j

i

ji

ji

jiC

Cnk (6)

where *jik is the apparent ozone decay rate based on measurements i and j, ni-j is the

number of chambers between sample points i and j, (HDT)i-j is the net theoretical

hydraulic detention time between sample points i and j, and Ci and Cj are the ozone

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24

residual concentrations measured at sample points i and j. Equation 6 is

evaluated between sample points 1 and 2 and between sample points 1 and 3. The

average decay rate, *avgk , is the average of *

21k and *31k , provided neither value differs

from the average by more than 20%.

The ozone concentration at the inlet to the reaction zone is estimated based on the

concentrations measured at the three sample points. First, an inlet concentration is

estimated based on the average decay constant and the measured ozone concentration at

each sample point:

10

10

10*11in, 1

n

avgQn

VkCC (7)

20

20

20*2in,2 1

n

avgQn

VkCC (8)

30

30

30*3in,3 1

n

avgQn

VkCC (9)

In equations 7-9, Cin,i is the reaction zone inlet concentration estimated based on the

concentration measured at sample location i, Ci is the concentration measured at sample

location i, iV 0 is the reactor volume between the reaction zone inlet and sample location

i, in 0 is the number of chambers between the reaction zone inlet and sample location i,

and Q is the volumetric flow rate. Concentration at the intake to the reaction zone is then

3

in,3in,2in,1 CCCCin

(10)

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25

The characteristic concentration for each chamber is calculated via the

expression

in

i

iavg

ini

nk

CC

0

0

0* HDT1

(11)

and the Ct for each chamber is the product of the hydraulic detention time and the

characteristic concentration for that chamber. The overall Ct for the reaction zone is the

sum of the Cts of the chambers in the reaction zone.

I.3.4 Roles for CFD within the Regulatory Framework

The models used to determine regulatory compliance are low-fidelity (zero-

dimensional) and were developed to be easy to use and very conservative in their

estimation of level of disinfection. Notwithstanding the presence of a CFD approach in

the current regulation, there are several roles CFD might play in the ozone contactor

design and benchmarking processes.

First, CFD models can provide detailed information on hydrodynamics that

cannot be deduced from tracer studies or from sampling from a small number of positions

in the reactor. This includes the situation where the reactor does not yet exist. Where

tracer studies might identify that short-circuiting is occurring, CFD could be used in

determining where the short-circuiting occurs. Where sampling such as that performed in

the extended CSTR analysis can provide information on ozone concentration at strategic

points, CFD can be used to predict concentration profiles anywhere in the reactor and

more accurately quantify the variations in concentration throughout the reactor. CFD

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26

might be used to inform the choice of sample locations, enabling engineers to

avoid regions of backflow or other regions where the concentration might not be

representative of reactor performance.

Second, CFD could be used as a component of the design process, supplementing

and guiding the more intelligent conduct of expensive and time-consuming

experimentation. If, through tracer analysis or other means, engineers determine a

reactor has an unusually short T10, they may opt to alter the reactor design to improve

hydraulics and achieve a higher Ct. A validated CFD could be used to predict

performance of reactors with modifications such as baffle additions, inlet or discharge

reconfigurations or modified sparger placement.

Finally, as is demonstrated in the dissertation, CFD can be used for modeling

multiphase reacting flows. This ability will enable design engineers to progress beyond

models in which the ozone transfer efficiency is assumed. Improved modeling and

understanding will yield reactor designs that improve bubble-liquid contact and mixing

and promote more uniform ozone concentration in the process water.

I.4 CFD in Water and Wastewater Treatment Operations Analysis

Computational fluid dynamics (CFD) is being used more frequently in the water

treatment and wastewater treatment engineering due to improvement in commercially-

available CFD codes (especially improved physics and chemistry submodels) and

because personal computers now have sufficient speed and memory to permit modeling

of realistic water treatment processes.

In water treatment, CFD has been used to

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27

assess design modifications for improved clarifier performance (Adams and

Rodi 1990; Lyn et al., 1992; Zhou et al., 1994; Brouckaert and Buckley 1999; Craig

et al., 2002),

simulate and troubleshoot flocculation processes (Ducoste and Clark 1999; Lainé et

al., 1999; Liu et al., 2004),

model the performance of a static mixer (Jones et al., 2002),

simulate hydrodynamics and microbial inactivation in pilot and full scale chlorine

contact chambers (Falconer and Ismail 1997; Wang and Falconer 1998; Greene et al.,

2001),

simulate multiphase flow in flotation processes (Sarrot et al., 2005);

assess ozone contactor hydraulics, mass transfer and microbial inactivation (Henry

and Freeman 1995; Murrer et al., 1995; Cockx et al., 1999; Do-Quang et al., 1999;

Cockx et al., 2001; Huang et al., 2002; Ta and Hague 2004) and

assess mixing in water storage tanks and reservoirs (Ta and Brignal 1998).

This list of applications will certainly grow as researchers develop and validate CFD

models for water treatment applications and the environmental engineering community

realizes benefits from CFD studies.

CFD has allowed engineers to perform relatively inexpensive testing and can be

used to assist in reactor scale-up and design (e.g., in design of a UV disinfection reactor

(Valade et al., 2003)). As noted in a previous study (Brouckaert and Buckley 1999),

treatment processes in water and wastewater treatment plants are often carried out in

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28

large vessels prone to non-uniform flow or other non-ideal flow characteristics.

Examples of non-ideal processes that may take place in typical unit operations are:

Short circuiting or dead zones in reactors;

Poor mixing of reagents (e.g., coagulants) in flow streams;

Inefficient settling in clarifiers operated at loadings different from design values;

Stratification in membrane reactors;

Stratification or short-circuiting in reservoirs and storage tanks.

Experimental determination of flow conditions in water and wastewater reactors and

appurtenances is costly given the size of reactors and the likelihood that units would have

to be taken off-line to facilitate measurements. Thus, CFD appears to meet a need

currently not addressed in the water treatment industry.

I.5 Need for the Current Study

As illustrated in the literature review below, current design methodology for

ozone contactors relies on simplified, calibrated models that are applicable over a

relatively narrow range of reactor designs and operating conditions. So the current study

was formulated to assess the ability of CFD to model operation of ozone bubble

contactors accurately, inclusive of all significant hydrodynamics, chemistry and biology,

using only submodels for turbulence (mixing), mass transfer, chemistry and microbial

inactivation that are independent of reactor geometry or operating conditions. Such a

capability would be a great benefit to engineers assessing the performance of pilot scale

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29

reactors and designing full-scale reactors in which hydrodynamics may differ

significantly from those encountered at the pilot scale.

Despite an extensive literature related to bubble columns, relatively few studies

have been conducted on the behavior and modeling of countercurrent bubble flows and

the performance of countercurrent bubble columns and even fewer have considered mass

transfer; to date the majority of published studies on bubble contactor operation have

focused on hydrodynamics and have analyzed columns of bubbles injected into a non-

flowing liquid column or cocurrent flow. The work performed in this study was

developed to advance the state of CFD analysis of bubble columns by adding the

complexities of countercurrent flow, mass transfer, reaction and microbial inactivation.

These additions are significant since the objective of a bubble column is to produce

efficient mass transfer between phases and contact between disinfectant and pathogenic

organisms and because many industrial bubble columns are run in countercurrent mode.

Just as a systematic study has been made of CFD submodels for momentum

exchange between phases, so should there be a systematic study of mass transfer models.

The CFD studies identified in the literature survey of this proposal present no strong

justification for their selection of mass transfer submodel and the scientific community

will benefit from a thorough review of the sensitivity of CFD simulations to choice of

mass transfer relation and guidance in selecting a relation for a given design and

operating condition.

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30

I.6 Significance of the Proposed Work

I.6.1 Advancement of Knowledge

The current work is intended to yield three important contributions to the

technical literature:

Rigorous verification and validation of CFD countercurrent hydrodynamics and mass

transfer submodels for ozone bubble contactor simulations;

Detailed experimental and modeling investigation of interphase ozone mass transfer

and mass transfer models; and

Demonstration of simultaneous prediction of microbial inactivation and bromate

formation with a CFD model that does not need to be “calibrated” with experimental

data.

The majority of bubble contactor CFD studies published to date have entailed modeling

hydrodynamics of bubble columns with either stagnant water or cocurrent flow. In the

few studies published that included interphase mass transfer, countercurrent flow and

microbial inactivation, researchers have not provided justification for their selection of

bubble drag, interphase mass transfer or microbial inactivation models. Validation of

submodels is an important step in demonstrating the utility of CFD in design of water

treatment unit operations and will boost the confidence of the water utility community in

CFD analyses.

Since bubble column hydrodynamics has been addressed in other studies, the

mass transfer studies proposed herein will likely yield the greatest immediate benefit to

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31

the scientific community. As described in detail below, mass transfer in bubble

columns is complex and varies with water depth within a given reactor operating at

known water and gas flow rates. The experimental work described below was designed

to allow visualization of the mass transfer process and yield quantitative and qualitative

data on the influence of phase distribution and mixing on the mass transfer rate. The

experiments were novel and, arguably, were a significant improvement over pilot reactor

mass transfer studies that have been performed in the past.

The CFD simulations of interphase mass transfer provide further details on

interphase mass transfer physics and, most important, demonstrate that CFD is a better

design tool than currently-used models and scale-up laws. CFD offers two benefits to the

other approaches:

Use of first principles in development of the model and

characterization of the problem in sufficient detail to account for the influence of

reactor geometry on reactor performance.

These benefits allow CFD to be used in more phases of the design process, even

including the design of pilot facilities. Whereas lower-fidelity models such as the one-

dimensional advection-dispersion-reaction model and completely stirred tank reactor

(CSTR) model require calibration and cannot be used for reactors whose geometry differs

from those to which the models were calibrated, CFD may be applied to any geometry.

Prediction of microbial inactivation and bromate formation in a full scale reactor

with a CFD model is significant both because it will be the first such study in a published

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32

work and because it will demonstrate a methodology for achieving an illusive

public health goal – balancing acute microbial risk with long term risk from DBP

consumption.

A final, incremental advancement in scientific knowledge is provided in

simulation of microbial inactivation in continuous flow reactors. The microbial

inactivation modeling performed builds upon the work performed by Greene (2003).

However, this work further develops a procedure for including microbial inactivation in

CFD simulations of continuous flow reactors and may expose alternatives or

modifications to the Ct approach to reactor design leading to reduced deleterious

byproduct formation.

I.6.2 Value to Industry

Compared with engineers from other disciplines, environmental engineers have

been slow to adopt CFD as a design and analysis tool, though in the past 3-4 years the

number of publications of CFD studies related to water and wastewater unit operations

has increased dramatically. Validation and experience with CFD such as demonstrated in

this dissertation should increase the confidence of the engineering community in CFD

analyses and demonstrate the utility of CFD to water utilities choosing between

experimental programs and CFD studies. CFD cannot replace careful experimentation in

water treatment. It can, however, be used in concert with experimentation to shorten

design cycle time, improve design of extant reactors, troubleshoot underperforming

reactors and explore novel reactor designs. This study can act as another stone in the

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33

foundation of studies that will make CFD a more attractive tool to

environmental engineers.

An additional value to industry of the current work is improved understanding of

ozone transfer in bubble contactors. According to calculations and experiments made in

this study and the observations made in past studies (Mariñas et al., 1993), the most

intense ozone transfer in bubble column reactors often takes place over a relatively small

vertical portion of the reactor. Most ozone contactors are designed for nearly 100%

ozone mass transfer efficiency (i.e., 100% of the applied dose transfer to the water). This

design philosophy is necessitated by the expense of generating ozone and a lack of design

relations capable of accurately predicting mass transfer rates in arbitrary geometries. The

insights into mass transfer drawn from the work reported in this thesis may suggest

reactor designs that are consistent with the processes occurring in countercurrent flow

mass transfer and achieve acceptable ozone transfer efficiencies with reduced bromate

formation.

The proposed work can contribute to the development and evaluation of the

models the U.S. EPA current allows for utilities wishing to claim inactivation credit for

ozone bubble contactors. Current guidelines do not allow inactivation credit for the first

chamber in which ozone is introduced into a bubble contactor. The assumption is that

ozone demand and decay in the first dissolution chamber are so high that no significant

accumulation of dissolved ozone occurs. CFD analyses, as performed in this study, could

allow detailed knowledge of ozone distribution in the first dissolution chamber and

assessment of this guideline. In addition, CFD calculations can be compared with results

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34

from CSTR, extended CSTR and segmented flow models of ozone bubble

contactors. These comparisons will provide information that will help utilities make

appropriate choices for modeling to claim inactivation credit and will provide

information to U.S. EPA on whether the segmented flow model is appropriate for ozone

bubble contactors and how best to apply it.

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35

II LITERATURE SURVEY

This chapter surveys studies of bubble column reactor hydrodynamics and

performance, ozone disinfection and byproduct formation, modeling studies apropos to

ozone bubble contactors and ozone bubble column reactor design and scale up.

First, a description of phenomena occurring in bubble column reactors in general

and ozone bubble contactors in specific is presented. Next, models for the physical and

chemical phenomena occurring in ozone bubble contactors are reviewed. This review is

merited since these models are employed in CFD simulations and because CFD

simulations may provide a means to estimate some of the parameters commonly used in

reactor design.

Significant processes that occur in diffused ozone bubble column reactors are:

Gas injection and bubble dynamics

o Introduction of gas into liquid stream

o Evolution of bubble shape and acceleration to terminal velocity

o Bubble breakup, collision and agglomeration

Mixing

o Large length scale liquid phase turbulence related to the reactor intake, discharge

and geometry and exchange of momentum between the bubble plume and liquid

outside the bubble plume

o Small length scale liquid phase turbulence related to dissipation of turbulence and

hydrodynamics of bubble wakes

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36

Mass transfer

o Dissolution of gaseous ozone molecules through chemical and physical barriers at

the bubble surface and into the liquid phase

o Diffusion (penetration) of dissolved ozone into liquid adjacent to the bubble

surface

o Exchange of liquid at the bubble surface with liquid from the bulk liquid phase

o Exchange of ozone-rich liquid in the bubble plume with ozone-poor liquid outside

the bubble plume.

Chemical reaction and microbial inactivation

o Ozone demand

o Ozone decay

o Bromate and disinfection byproduct (DBP) formation

o Microbial inactivation.

Studies that provide insight into or quantification of these processes are

summarized below. The data and relations presented are drawn from a rich literature on

bubble column reactors. The vast majority of published studies describe performance of

pilot scale cylindrical bubble column reactors operated in either co-current mode (with

the liquid and gas phases flowing in the same direction) or with non-flowing liquid phase.

Because bubble column reactor performance is strongly dependent on column geometry

(especially diameter to height ratio) and operating conditions (especially gas to liquid

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37

volumetric flow ratio), the studies summarized below should be applied to

countercurrent bubble column flow only after consideration of mode of operation and

scale.

After description of phenomena occurring in diffused bubble ozone contactors,

models that have been developed for bubble column reactors and ozonation processes are

summarized. Models differ in spatial dimensionality (0, 1 2 and 3 dimensional models),

type (empirical, stochastic and deterministic) and in the physics, chemistry and biology

included. Particular attention is paid to the application of computational fluid dynamics

(CFD) to bubble column reactors and to ozone bubble contactors.

II.1 Bubble Column Reactor Phenomena

Figure 5 is an illustration of the interrelated processes that occur in bubble

columns (Heijnen and Van't Riet 1984). As indicated in the diagram, flow and mass

transfer in bubble columns are related to the choice of sparger, liquid properties, gas

properties, bubble column operating conditions and bubble column geometry. Bubble

columns may be operated in co-current mode (with bulk gas and liquid flows in the same

direction), countercurrent mode (with liquid and gas phase bulk flows in opposite

directions) and without net liquid flow. Note that, even in the absence of net liquid flow,

bubbles produce large- and small-scale liquid motions in bubble columns. Dispersion,

hold-up and mass transfer differ significantly for bubble columns undergoing these three

modes of operation.

For all three modes of operation, changing the ratio of gas flow rate to liquid flow

rate changes the interactions between bubbles and between the phases. For relatively low

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gas flow rates and liquid flow rates less than the bubble terminal rise velocity,

bubbles tend to be small, non-interacting and dispersed and flow is in the “ideal bubbly

flow” or “dispersed flow” regime. In this regime, bubbles tend to be monodisperse and

there is not significant breakup or coalescence of bubbles.

Figure 5: Interrelated Processes in a Bubble Column (adapted from Heijnen andVan't Riet (1984))

II.1.1 Countercurrent Two-phase Flow Modeling

Depending upon the relative velocity of the phases in a countercurrent bubble

column, three flow regimes are possible: bubble flow (also called ideal bubbly flow);

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39

churn turbulent flow; and bubble down flow (Uchida et al., 1989). Bubbly flow

is characterized by a narrow, monomodal distribution of bubble diameter and negligible

break-up or coalescence (Olmos et al., 2003). Churn turbulent flow and the transition

region between bubbly flow and churn turbulent flow are also termed heterogeneous

flow. Homogeneous and heterogeneous bubble flows are illustrated in Figure 6. Other

regimes (churn turbulent and slug flow) may be encountered at very high gas flow rates,

but are not depicted in Figure 6 because it is unlikely they would be encountered in

typical ozone contactor bubble column operation.

Figure 6: Illustration of Homogeneous and Heterogeneous Bubbly Flow (Camarasaet al., 1999)

Bubble column flow regimes are shown schematically in Figure 7 (adapted from

Uchida, Tsuyutani et al. (1989)). The trends depicted in Figure 7 are based on

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40

experimental data collected for a single bubble column (4.6 cm inner diameter)

operated in countercurrent mode over a range of gas to liquid flow ratios. Data were

collected for air bubbled into water and glycerol solutions of 5%, 10% and 15%.

The transition from bubble flow (ideal bubbly flow) to churn turbulent flow

occurred in a well-defined band (depicted with dashed lines) of gas-liquid flow ratios for

the liquids studied. The transition from bubble flow to bubble downflow was, not

surprisingly, strongly dependent on liquid composition (and surface tension, which

influences bubble shape and surface mobility) and temperature. The family of solid

curves drawn on Figure 7 indicates the transition associated with the liquids tested.

Transition occurred earliest (at the lowest gas flow rate) for the 15% glycerol solution

and latest (at the highest gas flow rate) for the lowest-temperature water tested.

Based on their results, Uchida, Tsuyutani et al. determined that the boundary

between churn turbulent flow and other flow regimes was insensitive to the composition

and properties of the liquid phase and dependent mainly on reactor design and choice of

sparger. The boundary between ideal bubbly flow and bubble down flow was strongly

dependent on the composition of the liquid phase. This may be due to differences in

properties in the liquid phase and/or differences in bubble properties and tendency to

coalesce. Lockett and Kirkpatrick (1975) suggest that the transition from ideal bubbly

flow to churn turbulent may be related to liquid circulation due to spatial variations in gas

phase holdup at a given axial location or the presence of large bubbles. Flooding (not

shown on Figure 7) is unlikely for the flow conditions typically encountered in bubble

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41

columns and likely plays no role in the transition from ideal bubbly flow to

churn turbulent flow.

Figure 7: Countercurrent Bubble Column Flow Regimes Schematic Diagram(adapated from Uchida, Tsuyutani et al. (1989)

Ruzicka, Drahoš et al. (2001) quantified the effect of liquid depth and bubble

column diameter (for cylindrical columns) on the critical gas hold-up (column volume

occupied by gas divided by column volume) at which transition from homogeneous

bubbly flow to heterogeneous regime occurs. Although their work was done in bubble

columns with stagnant liquids, it can be assumed that transition from ideal to churn

turbulent flow in countercurrent bubble columns is also dependent on column diameter

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42

and liquid depth. In general, the authors found that increasing the column

diameter caused transition to heterogeneous bubble flow at lower void ratios and

increasing liquid depth in the column caused transition to heterogeneous bubble flow at

lower void ratios. In reviewing bubble column transition literature, Ruzicka et al. found

the effect of column diameter on transition was due to turbulence scale, intensity of

circulations, back-mixing, dispersion, wall friction and turbulent viscosity. The

dependence of liquid depth on critical void ratio was attributed to the relative importance

of the flow regions at the top and bottom of the column (compared with the region in the

middle of the column).

As described by Camarasa, Vial et al. (1999), the behavior and modeling of

liquid-solid two phase systems is significantly different from that of gas-liquid two-phase

systems. In gas-liquid two-phase systems, the properties of the dispersed phase (bubble

shape and size, distribution of bubbles in the column, influence of bubbles on each other)

depend on reactor geometry and operating conditions and the physico-chemical

properties of the continuous phase. According to Camarasa, this coupling of dispersed

phase properties with continuous phase behavior precludes a priori bubble column

reactor design given current knowledge of processes in bubble columns. Based on these

considerations, hydrodynamics and mass transfer are likely fundamentally different in

cocurrent bubble columns, countercurrent bubble columns and bubble columns in which

gas is introduced into non-flowing liquids. Specifically, liquid-phase dispersion,

circulation in the bubble column and bubble breakup and coalescence differ significantly

between the column configurations.

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43

Cocurrent bubble column flow has been studied in greater depth than

counter current bubble column flow. For example, Deckwer, Burckhart et al. (1974)

performed cocurrent flow experiments in bubble columns of 15 cm and 20 cm and

employing different spargers. The experiments were conducted with air bubbled into tap

water and various salt and molasses solutions. The primary objective of these studies

was development of relations to predict oxygen mass transfer. Based on measured gas

phase holdup and analysis of samples taken at an unspecified number of axial locations in

the reactor, the authors concluded that, for the cocurrent configuration employed,

there was little or no axial variation in oxygen mass transfer rate in the columns;

the mass transfer rate was influenced more by sparger type than column dimensions;

for the liquids studied, the mass transfer rate, kLa, varied roughly linearly with gas

velocity

addition of electrolytes to the solution appeared to reduce bubble size (increasing

specific surface area, a) but decrease mass transfer coefficient, kL, resulting in a

slightly lower overall mass transfer rate.

II.1.1.1 Bubble Size and Interfacial Area

The shape of bubbles and the drag they impart on the water depends upon the

water surface tension (which may, in turn, depend on the concentration of impurities in

the feed water), the manner in which they are injected into the water (gas flow rate and

diffuser type), the flow rate of the water column, and the temperature. Moore (1959)

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44

suggests that bubble shape is the dominant feature in determining bubble drag

and rise velocity in the flow regimes normally encountered in bubble column flows.

Bubble size is largely a function of sparger type, aqueous phase properties and gas

velocity. Though it is convenient to work with a characteristic bubble diameter in

performing calculations, it should be remembered that there is variation in bubble

diameter at a given axial station in a contactor and that bubbles change size in the

contactor, often having significantly different average diameter near the sparger

compared with mean diameter in the rest of the bubble column.

The two processes integral to determining bubble size are injection and

coalescence. Injection of gas into a liquid column may be via nozzles, porous discs or

two-phase injectors (Heijnen and Van't Riet 1984). The type of sparger largely

determines the size of bubble introduced to the liquid while the behavior and possible

coalescence of bubbles in the liquid column is mainly a function of aqueous phase

properties. Pure liquids tend to cause bubbles with more mobile surfaces that have a

greater tendency to coalesce. Less pure waters tend to produce smaller, more rigid

bubbles.

For relatively large-diameter bubble columns, interfacial area is usually

approximated by (Roustan et al., 1996):

g

g

bda

1

6(12)

where a is specific surface area (net surface area per reactor volume), db is effective

bubble diameter (diameter of a spherical bubble whose volume is the same as that of the

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45

bubble) and g is gas phase holdup (i.e., the gas phase volume divided by the

total reactor volume). For very small gas holdup, interfacial area can be approximated

by

a 6 g

db

(13)

For smaller-diameter columns, the column geometry may influence gas holdup and Akita

and Yoshida (Akita and Yoshida 1974) propose the relation

13.11.05.013.1

1.0

2

35.02

3

1

3

1gaog

L

cLcc GB

dgdgda

(14)

where dc is column diameter, g is gravitational acceleration, L is liquid phase density,

is surface tension, L is liquid phase kinematic viscosity, Bo is Bond number and Ga is

Galileo number. The Akita-Yoshida relation was developed based on analysis of data

from a 2.5 m high rectangular cross section bubble column outfitted with a porous plate

sparger.

Many relations have been proposed for bubble diameter, some of which are

presented in Table 5. These relations must be used with care. First, the relations predict

a single diameter bubble though in reality spargers discharge bubbles with a range of

diameters. Second, small differences in sparger manufacture, fouling of sparger or

corrosion may significantly alter discharge bubble diameter. Finally, relations are

generally derived for bubbles either at the sparger discharge or far enough into the liquid

column that coalescence and other changes are complete and a uniform, steady diameter

is established. Choosing just one of these locations as representative is a simplification.

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46

Gas phase holdup is another important design variable because it relates

to the overall transfer area, because it provides an indication of the bubble flow regime in

which the column is operating and because it is relatively easy to measure. As with

relations for bubble diameter, numerous relations have been developed for gas phase

holdup. Gas phase holdup relations that have been proposed in the scientific literature

and are applicable to ozone bubble contactor operation are summarized in Table 6.

Because many of these relations were developed based on empirical measurements care

should be taken to understand the conditions for which the relations were developed

before they are used.

.

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Table 5: Summary of Bubble Diameter Relations

Expression Source Sparger Location Notes

db 0.0287 do

1 2 Reo1 3 Reo 2100

0.0071 Reo0.05 10,000 Reo 50,000

Leibson inBenitez (2002)

Any with spacingbetween nozzles > 3 do

Sparger Based on air-water system data. Units ofand do are m.

db

1.7 do

r

1 3

Single bubble regime

1.17(U go ) do

0.8g 0.2 Continuous chain regime

4 mm db 6 mm Jet regime

Heijnen andVan't Riet(1984)

Nozzle Sparger In SI units. Single bubble, continuouschain and jet regime correspond toconditions at low, medium and high gasflow rates, respectively.

db

0.0061 U go do

0.1

d00.08

w

0.38

Coalescing

0.0104 U godo

0.1

d00.07

w

0.0.41

Non - coalescing

Heijnen andVan't Riet(1984)

Porous disc Sparger SI units. The ratio /w is the liquidsurface tension to pure water surfacetension ratio

0.5 mm db 1.0 mm Non -coalescing media

4.0 mm db 6.0 mm Coalescing media

Heijnen andVan't Riet(1984)

Injector/ ejector Sparger

47

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48

Expression Source Sparger Location Notes

db 4.15 0.6 g

0.5

v b

L

0.2

9.0104 m

Qg Patm lnPatm

Psp arger

v b 2

L db

0.5g db

1 2

Dudley (1995) Any Column is gas power input, vb is bubble free

rise velocity. Developed for turbinecontactor but widely used for bubblecolumns

db 2.15103 L gU g 0.16 Bín, Duczmal

et al. (2001)Porous plates Column Based on experimental data for large

bubbles in a bubble column. SI units,bubble diameter in mm.

48

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49

Table 6: Summary of Gas Phase Holdup Relations

Expression Source Notes

g

1 g 4

dc2 L g

1 8

g dc3

L2

1 12U g

g dc

Akita andYoshida(1973)

According to Deckwer and Schumpe (1993) this relation provides a “reliableconservative estimate” of gas hold-up. For pure liquids and non-electrolytesolutions =0.2 and for salt solutions =0.25.

U g 1 g U L g Vb g 1 g 2.39 Lockett and

Kirkpatrick(1975)

Developed for 5 mm air bubbles in disperse bubbly flow (g < 0.3).

g 0.672 fU g

0.578L

4 g

L 3

0.131 g

L

0.062g

L

0.107 Hikita, Asai etal. (1980)

According to Deckwer and Schumpe (1993), this relation provides slightly betterholdup estimates than the Akita Yoshida relation because variations in gas phaseproperties are accounted for. The value of f is 1 for non-electrolyte solutions andis a function of strength for salt solutions.

g 1.07U g

2

g dc

Kawase andMoo-Young(1987)

Based on theoretical relations developed for Newtonian and non-Newtoniancontinuous phase. The relation shown is for air bubbles rising in water at 20C

U g

g

0.175 Bo1 8 Ga

1 12 Res1 2 g dc

1 2

3.5103 Bo3 4 Res

2 7 1 0.85 g U L U g

Res db U s

L

U s U g

g

U L

1 L

Uchida,Tsuyutani etal. (1989)

Developed for countercurrent bubble flow in a variety of gas-liquid systems. Thisis the only relation identified that directly accounts for the difference betweencountercurrent and other bubble columns.

g U g

0.3 2U g

Langlais,Reckhow etal. (1991)

Assumes bubbles are free-moving and non-coalescent. Based on work byHughmark. 49

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50

Expression Source Notes

g C U gx

C x Sparger Column diameter

3.61 0.91 Porous plate 0.15 m

4.25 0.99 Membrane 0.15 m

3.66 0.83 Perforated Plate 0.15 m

3.43 1.03 Porous plate 0.2 m

3.12 1.05 Membrane 0.2 m

2.2 1.06 Porous plate 0.2 m

Bouaifi,Hebrard et al.(2001)

Given the clear dependence of gas holdup on column geometry and sparger type,this relation does not appear general. Units of superficial gas velocity in thisrelation are cm/s.

50

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51

II.1.1.2 Interphase Momentum Transfer

In his comprehensive article on bubble behavior, Moore (1959) described bubble

behavior (shape, rise velocity and drag) for bubbles in various liquids and with various

shapes. The parameters governing bubble drag and terminal velocity include liquid

properties (viscosity, density, surface tension, temperature), gas properties (viscosity,

density, surface tension), bubble diameter (which is largely a function of sparger type and

the tendency of bubbles to coalesce) and local acceleration due to gravity. Gas properties

are generally unimportant in determining bubble drag and rise speed. The remaining

parameters can be grouped and described via the dimensionless parameters, listed in

Table 7. Among the parameters making up the dimensionless quantities in Table 7, the

only one over which designers have substantial control is the bubble diameter.

Table 7: Dimensionless Parameters Associated with Bubble Drag and TerminalRise Speed

Name Formula Description

Mortonnumber 32

4

L

o

gM

Morton number is solely a function of liquid properties.Liquid to liquid variations are largely due to differences inviscosity, since surface tension is less variable. LowMorton number fluids are those with Mo < 10-8 and highMorton number fluids are those with Mo > 10-3. Pure waterhas Mo = O(10-10). The precise value depends upon thetemperature and purity of the water. In most casescontaminated water has a higher Morton number (due tothe presence of surface active agents and lower surfacetension) than pure water.

Reynoldsnumber Re

dbVb

L

The ratio of inertial forces to viscous forces. For bubbles,the characteristic length is the effective bubble diameter,defined as the diameter of a sphere whose volume is thesame as that of the bubble. The characteristic velocity isthe bubble terminal rise velocity.

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52

Name Formula Description

Webernumber We

db Vb

2

The ratio of hydrodynamic forces to surface tension forces.Where surface tension forces dominate (low Webernumber), bubble shape is that which minimizes surfacetension forces and is spherical. Where hydrodynamicforces dominate, the bubble assumes a shape to minimizedrag.

Eötvösnumber

2b

o

dgE

The ratio of gravitational forces to surface tension forces.

The significance of the bubble diameter and shape in determining bubble drag and

rise velocity is illustrated in Figure 8 (Moore 1959). For small bubble diameters

(generally less than 2 mm for air bubbles in water), bubbles are spherical and rise

rectilinearly. As bubble diameter increases, hydrodynamic forces play an increasing role

in determining bubble shape and bubbles assume ellipsoidal then oblate shapes. As

bubble diameter is further increased, bubble shape fluctuates and trajectories become

zigzag or spiral as bubbles ascend. In this Weber number range, the bubble rise speed

decreases significantly. At what is presumed to be a critical Weber number (Moore

1959), the trailing edge of the bubble becomes unstable in shape and bubbles assume a

spherical cap (mushroom-like) shape. In this regime, the leading (upward) edge of the

bubble has a stable hemispheric shape and a well-defined boundary layer. The rear

surface fluctuates in shape and the local flow field is dominated by turbulent eddies.

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53

Figure 8: Bubble Rise Velocity and Discharge Coefficient Schematics (Moore 1959)

Based on the forgoing, care must be used in choosing a drag coefficient relation

consistent with the bubble shape (Weber number regime) encountered in a bubble

contactor. Numerous relations have been proposed and used. The most commonly used

relations describing drag and terminal bubble speed of dispersed bubbles in a liquid

medium are presented in Table 8 and Table 9.

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54

Table 8: Summary of Bubble Drag Relations

Relation Source Notes

Various Stokes relation fora sphere risingsteadily at lowReynolds number.

SchillerandNaumann(in Clift,Grace etal. (1978))

For sphericalbubbles rising inthe viscousregime (Re < 800)and widelydispersed in aliquid.

Moore(1959)

Theoreticallybased relations forsingle bubblesrising in stagnantliquids.

C D

24

Re

Stokes regime

24

Re

1 0.1Re0.75 Viscous regime

2

3Eo

1 2117.67 f g

6 7

18.67 f g

2

Distorted particle regime

8

31 g

2Churn turbulent regime

f g 1 g

c

m

Ishii andZuber(1979)

For groups ofbubbles in allflow regimes.Relations aretheoretical andvalidated viacomparison withdata collected bymany researchers.Relations for dragin the distortedparticle and churnturbulent regimesare reported validto gas holdups of0.95. Reynoldsnumber based onbubble diameterand speed of thebubbles relative tothe liquid phase.

C D 24

Re

687.015.0124

e

e

D RR

C

C D

32

Re

Spherical bubbles, high R e

6

183 5M 1 5 W 3 5 Non - spherical bubbles

2.6 Spherical cap bubbles

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55

Relation Source Notes

Ihme inClift,Grace etal. (1978).

For rigid sphereswith Re < 104.

C D 4

3

g db

v b2

L

v b L

L db

M o0.149 J 0.857

3.5942.3

3.59294.0441.0

751.0

J

ref

149.0

3

4

Loo ME

Grace (inClift,Grace etal. (1978))

For distorted airbubbles rising inwater. Referenceviscosity is that ofpure water atspecifiedtemperature andpressure and canbe taken as0.0009 kg m-1 s-1.Valid over therange of specified.

36.048.524 573.0

ee

D RR

C

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56

Table 9: Summary of Bubble Terminal Speed Relations

Expression Source Notes

L

eBBL

Be

Be

L

Be

BeL

BeBeL

Be

L

GLBe

B

dVR

where

RMg

MRMR

MRRg

RgR

V

,

,

,

25.0

1

25.0

25.0

1,

214.0

1

5.0

,

214.0

1,

28.1

,

52.076.0

,

2

,

10.318.1

10.302.435.1

02.4233.0

29

2

Peebles andGarber(1953)

The variable dB,e is theeffective bubble diameter(the diameter of thesphere that has the samevolume as the bubble) andthe variable M is theMorton number.

VB L

L db

M o0.149 J 0.857

J 0.940.747 2 59.3

3.420.441 59.3

4

3Eo M o

0.149

Clift, Graceet al. (1978)

For single ellipsoidalbubbles rising incontaminated water.Validate for Mo < 10-3, Eo

< 40, Re > 0.1 andaqueous viscosity notsignificantly differentfrom that of pure water.

VB 2 g

L2

1 4

1 g 1.75

Ishii andZuber (1979)

For bubbles in liquids inthe distorted particleregime.

VB 0.574

g

U g

g dc 0.5

2.5 Viswanathanand Rao (inKawase andMoo-Young(1987)

Theoretically-derivedrelation that includesdependence on columndiameter.

VB

210db

1.004

L

0.5 db 1.8mm

20 33.8e4.88db 1.004

L

1.8 db 4mm

Mariñas,Liang et al.(1993)

Empirical relation basedon observations of the riseof single bubbles instagnant liquids. Units ofVB, db and L are cm/s, cmand centipoise,respectively.

VB 2

db

0.5g db

Winkler (inDudley(1995))

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57

II.1.1.3 Bubble-Induced Turbulence

Bubbles generate turbulence in their wakes, the practical results of which are

altered drag on other bubbles and changes in mixing. Sato and Sekoguchi (Sato and

Sekoguchi 1975) proposed a turbulence model that accounts for the fact that bubbles in a

shear flow (such as in a turbulent eddy) generate their own turbulence due to form drag.

The authors proposed that instantaneous fluid velocity in a bubble-laden flow can be

expressed as:

V V

V

V (15)

where

V is local instantaneous fluid velocity, V

is fluctuating velocity component

(instantaneous turbulence velocity) inherent in the liquid and independent of the

existence of bubbles and V

is a fluctuating velocity component caused by the motion of

the bubble relative to the surrounding fluid. As with single-phase turbulence modeling,

the velocity expression is introduced into the liquid phase momentum equation and the

resulting equation is averaged. This procedure produces an additional viscosity term in

the momentum equation:

eff L T B,T (16)

where eff is effective viscosity, L is liquid molecular viscosity, T is turbulent viscosity

and T,B is bubble-induced turbulent viscosity. This relation is available as an option in

the commercial CFD code that has been used in numerical simulations in this work.

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58

II.1.1.4 Mixing

II.1.1.4.1 Large Scale Hydrodynamics and Mixing

Mixing is critically important in ozone bubble columns. Small scale mixing

(dispersion) renews bubble surfaces with low ozone content liquid and promotes mass

transfer. Dispersion also carries water with high dissolved ozone concentration into

water with low ozone concentration

Mixing in ozone bubble contactors depends on the gas and liquid flow rates in the

contactor and the contactor geometry (Schulz and Bellamy 2000). Properly designed and

mixed operations do not have significant “channeling (short-circuiting)” or temporal

variations in ozone residual at a given location for a given gas and liquid flow rate.

Mixing in industrial ozone facilities is most often assessed based on the coefficient of

variation of time series of ozone residual at the reactor discharge. A coefficient of

variation less than 5% is thought to indicate sufficient mixing and that short-circuiting or

other non-ideal hydrodynamic processes are not significant (Schulz and Bellamy 2000).

When mixing in an ozone bubble contactor is believed to be inadequate, the most

common remedial actions are:

addition of ozonated air or oxygen at a lower ozone concentration and a higher gas

flow rate;

ensuring a dense coverage of diffusers in chambers where gas is introduced;

supplemental mixing with diffused air or water jets;

improvement of intake or discharge hydraulics.

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59

Because design data and guidelines for implementing these changes are not available,

experience is the only guide to effective choice and design of appurtenances for

enhancing mixing.

Large scale mixing phenomena determine how well the phases are distributed in a

reactor and the likelihood of short-circuiting or backmixing in the reactor. Bubble

plumes tend to migrate to walls or toward each other, as shown in Figure 9 and Figure 10

(Freire et al., 2002). This effect, sometimes called the Coanda effect, arises because

entrainment of liquid into the bubble plume is constrained on one side.

Figure 9: Migration of a Bubble Plume to a Wall (Freire et al., 2002)

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60

Figure 10: Migration of Bubble Plumes toward Each Other (Freire et al., 2002)

In ozone bubble contactors, bubble plume migration may occur, depending on

sparger placement and gas to liquid flow ratio. Depending on the type of feed for the

ozone generator (oxygen or air) and the design gas flow rates, rod and dome shaped

diffusers may be used in full scale fine bubble contactors. Rod shaped diffusers are

usually used when air is ozone generator feed gas and gas flow rates between 0.057 and

0.17 m3/min (2 and 6 ft3/min). Dome shaped diffusers are most often used when oxygen

is the feed gas and gas flow rate is between 0.014 m3/min and 0.17 m3/min. A guideline

for sparger spacing 4 ft2 or less per diffuser (Rakness 2005).

Numerous studies have been made of large-scale mixing in bubble columns with

non-flowing liquid phase (Grevet et al., 1982; Anderson and Rice 1989; Drahos et al.,

1992; Burns and Rice 1997; Lapin et al., 2002) but only one (published in multiple parts)

was identified that described or quantified large scale mixing in countercurrent flow

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61

columns (Anderson and Rice 1989; Burns and Rice 1997). In columns with non-flowing

liquid phase, bubble plumes entrain liquid as they rise, establishing regions of circulating

flow outside the bubble plume. The size and arrangement of these circulations is

dependent on the gas flow rate and the reactor geometry. Shallow bubble beds (height /

diameter 2) with non-flowing liquid phase establish a single circulation cell outside the

bubble plume. Bubble beds with larger height to diameter ratios establish multiple cells

(Drahos et al., 1992).

In countercurrent flow in cylindrical reactors, liquid flow tends to be upward in

the “core” of the bubble plume, and downward outside the bubble plume near the wall

(Burns and Rice 1997). The presence of a strong liquid down flow outside the bubble

plume reduces the amount of recirculation in the liquid phase. At high gas to liquid flow

ratios (but below churn turbulent flow) the bubble plume tends to grow in diameter more

slowly as it rises compared plumes at lower gas to liquid flow ratios.

For tall cylindrical bubble columns, minor misalignments of the centerline from

vertical can result in drastic differences in liquid flow (Rice and Littlefield 1987). In the

cited study, the authors filled a cylindrical bubble column with a solution of hydrochloric

acid and a pH indicator, sparged air into the solution until steady state hydraulics were

achieved, then pumped a strong solution of sodium hydroxide into bottom of the reactor.

As the sodium hydroxide progressed upward in the reactor, the pH indicator changed

color. Near the sparger the reactor behaved like a continuously stirred tank reactor

(CSTR) and the progress of the line of neutralization could not be followed. Above the

entrance region, the line of neutralization between the acidic and basic regions tended to

be distinct and to rise steadily. The progress of the line of neutralization was recorded on

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62

video tape. The rate of rise of the line of neutralization was computed from the video

images and the liquid phase dispersion was calculated via fitting a one-dimensional axial

dispersion model to observed rates. Two findings drawn from that study are of

importance to the current study. First, minor vertical misalignments (less than 0.5°) of

the column from true vertical resulted in major differences in dispersion. Second, an

“entrance region” was determined to exist near the sparger. This entrance region behaved

as a plug flow reactor. Regression was used to determine model parameters (dispersion

and height of the entrance region) that best fit experimental data. Unfortunately the

authors did not report the dependence of the height of the entrance region on gas flow

rate.

II.1.1.4.2 Small Scale Hydrodynamics and Mixing

Bubbles give rise to liquid-phase hydrodynamic dispersion in bubble columns and

dispersion, in turn, influences mass transfer rates. To date most analyses have

approximated liquid dispersion in a bubble column via a single dispersion number

(inverse of Peclet number) though dispersion likely varies axially in bubble columns. For

example, in a study of cocurrent air-water flow in bubble columns, Deckwer, Burckhaart

et al. (1974) found that dispersion was lower in the vicinity of the sparger compared with

dispersion in the rest of the column. In a study of a bubble column with no net liquid

flow, other authors determined the region near the sparger behaved as a CSTR (Rice and

Littlefield 1987).

Lehrer (1984) identifies the following parameters as influencing dispersion:

Gas and liquid flow rates;

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column dimensions;

configuration of fluid injection; and

properties of fluids.

Based on these observations, the author proposed a relation for axial dispersion of the

form:

EL EBB EK i

i1

N

QbU g (17)

where EL is the axial dispersion, EB is the contribution due to bubble form drag, B is a

hindered motion factor which accounts for interactions between bubbles, EK is the

contribution due to fluid injection through sparger holes, N is the number of sparger

holes, Qg is gas volumetric flow rate and Ug is gas superficial velocity. This relation has

limited applicability, given that for high gas flow rates the turbulent dispersion can

decrease or even become negative.

A number of relations for liquid phase dispersion commonly cited in the literature

are provided in Table 10. The conditions under which data supporting these relations

were taken are provided in the notes. These conditions should be given careful attention

given the importance of sparger type and reactor geometry in dispersion.

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Table 10: Axial Dispersion Relations

Relation Source Notes

EL 2.7 d c1.4 U g

0.3 Deckwer,Burckhart etal. (1974)

Developed for cocurrentflow of air in water,molasses and salt solutionsin two cylindrical bubblecolumns of 15 and 20 cmdiameter and 4.4 and 7.23 mwater column heights. Unitsof column diameter, dc, andsuperficial gas velocity, Ug,and liquid phase dispersion,EL, are cm, cm/s and cm2/s,respectively.

315.190.0 sggcL UUHdE Field andDavidson(1980)

Developed for cocurrentgas-liquid flow with Ug >>UL. In this equation Us isslip velocity and units arem2/s, m, m, m/s and m/s forEL, dc, H, Ug and Us,respectively.

EL 1.3134g 0.2 N 0.2 Qg0.6 tanh

0.168g 0.2 dc

N 0.3 Qg0.4

1 2

QU g

Lehrer(1984)

Theoretical relationdeveloped based on energyimparted to the liquid streamby gas injection, bubble dragand friction on columnwalls.

67

35

21

1 7.900185.088.4

b

L

L

g

edU

U

Hp

Kim,Tomiak etal. (2002a)

Developed based onexperimental observation inright circular cylindricalbubble columns. Units ofcolumn height, H, are m.Units of other variables mustbe dimensionally consistent.

6.03231

1.0

123511

3.1

areg

e

c

eGFR

R

d

HP

Moustiri,Hebrard etal. (2001)

Developed for cocurrentgas-liquid flow incylindrical columns. Theauthors found a pronouncedeffect of column diameter,fluid superficial velocitiesand bubble regime ondispersion.

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II.1.1.5 Interphase Ozone Mass Transfer

The first step in the dissolution of an ozone molecule is transport of the molecule

from the bulk gas phase (interior of a bubble) to the gas-liquid interface. As the ozone

molecule approaches the interface, it encounters resistance to its transport. This

resistance is a result of forces between gas and liquid molecules at the bubble surface and

additional forces related to the accumulation of surface active agents at the bubble

surface. These surface active agents accumulate as bubbles rise, explaining, in part, the

dependence of mass transfer rate on bubble age or reactor height. Surface active agents

are thought to produce interfacial resistance through formation of an energy barrier,

formation of a physical “sieve” that blocks some gas molecules or by influencing small

length scale hydrodynamics near the bubble surface (Goodridge and Robb 1965;

Vasconcelos et al., 2002; Alves et al., 2005).

At the bubble length scale, features that influence mass transfer are the shape of

the bubble, fluid motion on the length scale of the bubble diameter and proximity of other

bubbles. As illustrated, to accurately predict mass transfer, one must account for bubble

surface area (shape and effective diameter), gas phase hold-up, gas phase distribution,

liquid phase dispersion and circulation and chemical properties at the bubble surface.

Along with mass transfer, there is momentum transfer between the gas and liquid

phases. Momentum transfer results in enhanced turbulence and may lead to an increase

in dispersion and mixing, though not necessarily. In bubble columns and other

multiphase mass transfer operations, efficient mass transfer is facilitated by contacting

the phases in such a way that the difference in concentration of the material that is

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66

transferred is a maximum. So, countercurrent bubble columns (in which the liquid flows

downward and the gas bubbles upward) are preferred over cocurrent configurations.

Since the early 20th century, numerous researchers have sought to identify the

features that govern mass transfer between bubbles and liquids and have proposed

relations to predict the rate of transfer. The features that may govern mass transfer have

been identified as:

The manner in which bubbles are introduced into the contactor;

Liquid physical properties (viscosity, surface tension and dissolved ozone diffusivity;

The superficial gas flow rate;

The rate of dissolved ozone consumption in liquid phase reactions;

The presence of surface-active contaminants;

The contactor geometry (especially the ratio of the diffuser area to the contactor cross

sectional area and diffuser height); and

Bubble age.

Table 11 summarizes dimensionless parameters for characterizing bubble column mass

transfer.

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67

Table 11: Dimensionless Parameters Relevant to Bubble Column Mass Transfer

Dimensionless parameter Formula

Bond numberBo

g dc3 L

Froude numberFr

U L2

g d c

Galileo numberGa

g dc3

L2

Peclet number

i

Bg

eD

dUP

Reynolds numberRe

U g db

L

Schmidt numberS c

L

D i

Sherwood numberS h

kL dB

D i

In development of early models of the dissolution of gases, it was hypothesized

that there are thin layers of stagnant fluid on both sides of the gas-liquid interface, as

illustrated in Figure 11. In order for a gas molecule to diffuse from the bulk gas phase to

the bulk liquid phase, it must first overcome the gas film resistance, the resistance of the

surface layer and the liquid film resistance. The flow in the gas and liquid films is

assumed laminar and flow in the bulk phases is usually assumed to be turbulent.

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Bulk gas phase

Gas film

Liquid film

Bulk liquid phase

Gas film resistance

Surface layer resistance

Liquid film resistanceL

Lk

R1

s

sk

R1

G

Gk

R1

Figure 11: Schematic Diagram of the Two-Film Mass Transfer Model

Surface resistance depends upon the composition of the gas and liquid phases and

the presence of surface active agents that accumulate at the gas-liquid interface. Surface

active agents are hypothesized to offer resistance to gas diffusion via (Goodridge and

Robb 1965):

development of an energy barrier that impedes the progress of low-energy gas

molecules;

a sieving effect caused by the collision of gas molecules with surface agent agent

molecules assembled at the gas-liquid interface;

alteration of the hydrodynamics and size of the gas and liquid films adjacent to the

gas-liquid interface.

Surface active agents alter mass transfer rates indirectly by influencing the nature of the

bubble surface and consequently the bubble size, shape and tendency to break up or

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69

coalesce with other bubbles. The presence of trace concentrations of surface active

agents tends to change the mobility of bubbles surfaces (Clift et al., 1978; Alves et al.,

2005), the effective bubble diameter and holdup observed at a given liquid and gas flow

rate (Anderson and Quinn 1970). In studies of carbon dioxide sparged into distilled

water, de-ionized water and tap water, bubble coalescence was significantly lower in tap

water than in either de-ionized water or distilled water (Anderson and Quinn 1970). The

authors attributed this finding to the presence in tap water of substances that decrease the

mobility of bubbles and the possible presence in trace concentrations of coalescence-

promoting substances (possibly from resins in deionizing filters) in distilled and

deionized waters. For the ozone-water system, the Henry’s law constant varies with pH

and ionic strength as well as temperature (Bín 1995). The impact of surface active agents

on mass transfer is profound – the rate of dissolution of gases into waters with very low

ionic concentration is more than twice that into tap water (Alves et al., 2005).

Surface active agents (Vasconcelos et al., 2002; Alves et al., 2005) and

microorganisms (Blanchard 1970; Wozniak et al., 1976) accumulate on bubble surfaces

as bubbles rise through contaminated liquids. This accumulation explains the observed

dependence of mass transfer on bubble age. In studies of bubble rise velocity and mass

transfer rates of single bubbles, the rise velocity and mass transfer rate were both found to

decrease as a function of time as surface active materials accumulated on the bubble

surface. Liquid side mass transfer coefficient was found to lie between the value

predicted by penetration theory (which assumes a completely mobile bubble surface and

is described below)

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70

b

sL

d

Duk 13.1mobile (18)

and that predicted for a bubble with a rigid surface

6132rigid 6.0 Dd

uk

B

sL (19)

In equations 17 and 18, us is slip velocity (relative velocity between the bubble and

liquid), D is molecular diffusivity, dB is bubble diameter and is dynamic viscosity of the

liquid phase. The phenomenon of bacterial accumulation on bubble surfaces does not

impact mass transfer, but does influence the transport of microorganisms and the

uniformity of their contact with disinfectant.

Mass transfer models proposed after the two-film model recognized that the gas

and liquid film are not likely to be stagnant. Rather, fresh liquid and gas are continuously

exchanged between the films and bulk phases. The hydrodynamics related to the

transport of ozone from bubbles to the bulk liquid phase are illustrated in Figure 12. At

the bubble scale, gas phase circulation within the bubble influences the distribution of

ozone in the gas phase, the shape of the bubble and the rate at which ozone is transported

from the bulk gas phase to the gas-liquid interface. In the liquid phase, small scale

turbulence present in the bubble wakes and generated via hydrodynamic dispersion

transport liquid from the bulk phase to the bubble surface. Large scale fluid structures

(with length scale equal to the bubble column diameter) advect dissolved gases away

from the bubble plume and, in the case of uneven distribution of phases, into the liquid

phase.

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71

Low ozoneconcentration

downwardflowing liquid

Ozone-rich liquid inthe bubble plume

Gas phasecirculation

Liquidrenewal atthe bubble

surface

Figure 12: The Hydrodynamics of the Transport of Ozone from Gas Phase to theBulk Liquid Phase

In the first mass transfer model proposed to account for realistic exchange of

liquid between the bulk phase and film (called penetration theory), it was hypothesized

that parcels of “fresh” liquid from the bulk phase are in contact with the interface for a

characteristic time (Higbie 1935). During the contact time between the fluid parcel and

interface, dissolved gases “penetrate” into the fluid parcel. Fluid parcels having longer

contact times with the bubble surface experience greater depth of penetration of the

dissolved gas into the fluid parcel. Dissolved gas penetrates into the fluid parcel fastest

during initial contact of the parcel with the bubble surface when the dissolved gas

concentration in the fluid parcel is low. After long contact times the dissolved gas

concentration in the fluid parcel increases and the flux of dissolved gas into the fluid

parcel decreases. Assuming negligible gas phase resistance to mass transfer, penetration

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theory predicts the absorption rate for fluid parcels with a contact time of with the gas-

liquid interface is given by

D

CC 0* (20)

where C* is gas phase concentration divided by Henry’s law constant, C0 is the initial

dissolved gas concentration in the fluid parcel and D is the diffusivity of the dissolved

gas in the liquid. Assuming the contact time between a fluid parcel and the bubble

surface is equal to the bubble diameter divided by the slip velocity, Higbie’s penetration

theory predicts the liquid mass transfer coefficient is given in equation 18 (repeated

below)

b

sL

d

Duk 13.1 (18)

Since the penetration theory was proposed, researchers have proposed alternative

mass transfer models in which the contact time between fluid parcels and the gas-liquid

interface is not uniform. Danckwerts (1951) suggested that fluid parcels are exchanged

randomly at the gas-liquid interface and that the overall mass transfer coefficient at a

given time is the integrated mass transfer to all fluid parcels (with a distribution of

contact times with the gas-liquid interface) at the interface. This model, in which parcels

are renewed at the interface with some distribution of parcel contact times, is called the

“surface renewal” model. These assumptions give rise to the mass transfer rate

sDkL (21)

where s is the random replacement rate for fluid particles at the interface (units of T-1).

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73

Although it may better reflect interface processes, relation 10 is used for

predicting mass transfer rate less often than equation 7, perhaps because of the difficulty

in estimating the replacement rate. Since the introduction of the surface renewal model,

other investigators have developed mass transfer models using various distributions of

parcel residence times at the interface. For example, a mass transfer model assuming the

distribution of parcel residence times at the interface was given by the gamma

distribution provided improvements in mass transfer prediction in turbulent pipe flow

over predictions based on Danckwerts’ model (Harriott 1962). Although the replacement

rate for parcels is likely related to the distribution of eddy sizes in turbulent flow, no

studies were found that related mass transfer coefficient to distribution of turbulent

kinetic energy.

The most commonly used relations for mass transfer are presented in Table 12.

The relations are presented as they were presented in original publications except where

the original nomenclature conflicts with that used in this dissertation. The basis

(theoretical, empirical and semi-empirical) for the relation and notes on the data on which

the relations were developed are also presented. Among the relations in Table 12, the

Hughmark relations (Hughmark 1967a; Hughmark 1967b) are most widely used and

basic mass transfer text books present them as the de facto standard for bubble contactor

design (Rakness et al., 1988; Benitez 2002). Although the Hughmark relations are

convenient to use and have long records of accomplishment, care should be taken in

choosing and using them – Hughmark’s original papers presented several alternate

relations appropriate for different flow regimes. The correct formula should be chosen

and justification should be provided for that choice.

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Calderbank and Moo-Young (1961) determined that the two most important

parameters in determining interphase mass transfer between dispersed bubbles and a

continuous liquid are diffusivity of the gas diffusing into the liquid and the size and flow

regime of the bubble. In general, mass transfer rates from larger bubbles is greater than

that from small bubbles, presumably because in large bubbles form drag predominates,

while friction drag predominates for small bubbles. The hydrodynamics associated with

friction drag present a barrier to penetration of dissolved gas into a continuous liquid,

while turbulent wakes behind large bubbles disperse dissolved gases away from bubbles

and bring low-concentration fluid in contact with the bubbles. Large diameter bubbles

were considered those with a diameter greater than 2.5 mm. Motarjemi and Jameson

(1978) validated the Calderbank and Moo-Young expressions for large and very small

bubbles, but found that in the transition region between small and large bubbles, the mass

transfer was significantly higher than that predicted by Calderbank and Moo-Young.

Their finding led them to propose an optimal bubble size of 1 mm for oxygen transfer in

air-tap water systems.

The debate over small and large bubble behavior should also consider the

presence of surface-active contaminants in the water and their effect on bubble size,

shape and behavior. Anderson and Quinn (1970) found a marked difference between gas

phase holdup and bubble shape between experiments with air bubbled in distilled water

and air bubbled in tap water. When bubbled in distilled water, air bubbles had a greater

tendency to coalesce and form spherical cap bubbles. In concluding, the authors caution

that trace amounts of contaminants may drastically change bubble column mass and

momentum transfer behavior and that, in conducting tracer experiments, care should be

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75

taken in choosing a tracer that does not have surface-active properties. Dudley (1995)

states that surfactants reduce surface tension, resulting in greater specific surface area.

However, surfactants also alter gas diffusivity in the aqueous phase and make bubble

surfaces more rigid. The net result of the presence of surfactants is a net reduction in kLa

in contaminated waters compared with transfer in pure water. Deckwer, Burckhart, et al.

(1974), like Dudley, noted that while specific surface area increases as surfactants are

introduced into the liquid phase, mass transfer coefficient, kL, reduces. This is attributed

to the formation of an electric double layer at the gas-liquid interface that impedes the

diffusion of dissolved gas into the aqueous phase. Prior researchers have suggested

mechanisms other than formation of an electric double layer to explain the way in which

surfactants impede mass transfer (Goodridge and Robb 1965). These mechanisms

including a “sieving effect” (physical entrapment of gas molecules by a thin surfactant

film) or hydrodynamic effects such as change in mass transfer boundary layer thickness

or local turbulence scale at the gas-liquid interface. In a recent study, it was suggested

that the major influence surfactant have on mass transfer relates to the impact of surface

active agents on bubble size and shape (Sardeing et al., 2006).

Dudley (1995) evaluated a number of mass transfer coefficient expressions

developed using a theoretical basis or data from co-current and non-flowing liquid bubble

columns (Calderbank and Moo-Young 1961; Motarjemi and Jameson 1978; Khudenko

and Shpirt 1986; Öztürk et al., 1987; Kawase and Moo-Young 1992) against

experimental mass transfer data collected in a 0.2 m diameter bubble column with a

height of 4 m and non-flowing liquid phase. Two diffusers of differing diameter and

unspecified type injected air into the columns. Liquid height, gas flow rate and liquid

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76

composition were varied. The relation providing the best correlation with the

experimental data was that of Kawase and Moo-Young (1992). Dudley recommends the

Kawase relation for general use because of its good correlation with data and its

theoretical basis.

Heijnen and Van’t Riet (1984) suggest the use of the Higbie relation for bubbles

of diameters larger than 2 mm in diameter. This suggestion is made based on analysis of

mass transfer data from many sources but is questionable given the tendency of

surfactants to make bubbles more rigid (more like small bubbles) and the conclusion of

Calderbank and Moo-Young (1961) that the transition between small and large bubble

behavior is for bubbles whose diameter is between 1 and 2.5 mm. The range of mass

transfer coefficients expected in typical bubble columns for bubbles of average diameter

greater than 2 mm is 2 10-4 m/s < kL < 3 10-4 m/s. For bubbles of average diameter

less than 0.8 mm the transfer coefficient is insensitive to bubble diameter and

approximately 1 10-4 m/s.

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7777

Table 12: Summary of Mass Transfer Relations for Dispersed Bubbles in Continuous Liquids

Author Relation Basis2 Description

Higbie (inMotarjemiand Jameson(1978))

kL 2

D i

te

2

D i U s

Lc

2

ReS c

Pe

T Developed based on penetration theory. The variable te is the time totraverse one bubble diameter and corresponds roughly to the contacttime between liquid fluid parcels and bubble surface. This relationwas proposed based on an assumption that form drag predominatesand bubble surface is mobile. The relation is most appropriatelyused for large bubbles.

Froessling (inMotarjemiand Jameson(1978))

S h 0.6 Re1 2 S c

1 3 T Developed from potential flow theory for small spherical rigidbubbles. This relation was proposed based on the assumption thatfriction drag predominates and mass transfer takes place through alaminar boundary surrounding the bubble. This relation is mostappropriately used for small bubbles.

Calderbankand Moo-Young (1961)

kL

0.31

L

gD i

S c

1 3

Bubble swarms, dB 2.5 mm

0.42

L

g 2Di

2

S c

1 6

Bubble swarms, dB 2.5 mm

E Correlations developed based on historical data and data collectedfor a variety of gas-liquid systems and with a variety of diffusers.The units of kL depend on the choice of units for g and Di. Figuresincluded in the paper indicate that small bubbles might be more-appropriately designated as those 1 mm or smaller in diameter.

Hughmark(1967b)

S h

2 0.6Re1 2S c

1 3 1 Re 450; S c 250

2 0.5Re1 2S c

0.42 1 Re 17; S c 250

2 0.4Re1 2S c

0.42 17 Re 450; S c 250

2 0.27 Re0.62S c

1 3 450 Re 104; S c 250

2 0.175Re0.62S c

0.42 450 Re 104; S c 250

E Developed based on mass transfer data from single, rigid spherestaken for a variety of species dissolving into a variety of liquids.

2 Designations are: “T” for theoretical, “E” for empirical and “SE” for semi-empirical (based on calibrated models developed from the Buckingham pi

theorem).

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7878

Author Relation Basis2 Description

Hughmark(1967a)

S h 2 a Re0.484S c

0.339 dB g1 3

D i2 3

0.072

b

a=0.061, b=1.61 for individual gas bubbles

a=0.0187, b=1.61 for bubbles in swarms

E Developed based on bubble column data from numerous sources andwith a variety of gas-liquid systems (CO2-water, Air-Water, Air-glycerol, air-aqueous solutions). Sherwood number is based onbubble diameter and dissolved gaseous species diffusivity.

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7979

Author Relation Basis2 Description

Lochiel andCalderbank(1964)

For rigid bubbles (fixed shape):

Sh

0.99Pe1 3 Re 1; spherical bubble

0.84 Re1 2Sc

1 3 Re 1; spherical bubble

Sh,sphereE2 2

3(1 k)

1 2

All Re , oblate spheroids

For bubbles with mobile interfaces,

Sh

0.65L

L G

1 2

Pe1 2 Re 1; spherical bubble

1.13 12.96

Re1 2

1 2

Pe1 2 Re 1; spherical bubble

Sh,sphere

2

31 k

1 2

All Re , oblate spheroids

Where

2E1 3 E 2 1

E E 2 1 ln E E 2 1 E1 6

k eE 2 Esin 1 e

eEsin 1 e

e 11

E 2

T Theoretical relations developed for high Peclet and Schmidt numbercases. Relationships were derived for single bubbles of knownshape. Relationships were also developed for spherical cap shapedbubbles, but these are not presented here because spherical capbubbles are unlikely to be encountered in ozone bubble contactors.

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8080

Author Relation Basis2 Description

Deckwer,Burckhart etal. (1974)

kL a b0 U gb1

where b1=0.0086 and b1 = 0.884 correspond to a 20 cmdiameter bubble column of total height 7.23 m outfittedwith 56 injector nozzles and b1=0.0274 and b1 = 0.8correspond to a 15 cm diameter bubble column of totalheight 4.4 m outfitted with 56 porous plate injector.

E Based on measurement of interfacial area and mass transfer incocurrent flow bubble columns of varying diameter and injectortype. Liquids in the bubble column were water, assorted saltsolutions and molasses. Oxygen transfer was observed and it isassumed that air was the dispersed phase gas.

Akita andYoshida(1974)

Sh 0.5 Sc1 2 Ga

1 2 Bo3 8 E Mass transfer and specific surface area data were collected in three

bubble columns. The columns had square cross sections and were2.5 m tall. The cylinder side dimensions for the three columns were7.7 cm, 15 cm, and 30 cm. Single orifice spargers were used for allthree columns and porous plate and perforated plate spargers wereused in the 15 cm column. Oxygen and air were employed as thedispersed gas phase fluid. Numerous liquids were used as thecontinuous fluid, including water, glycol solutions, glycerolsolutions, methanol and sodium sulfite solution.

Jackson andShen (1978)

kL

a 20

2.37 U g1.07H0.45 Based on previous data

2.28 U g1.14 H0.55 Based on 1.8m tank data

0.53 U g1.15 Data from all experiments

E Based on air bubbled into deoxygenated water or mixed liquor.Three tanks (76 mm, 1.8 m and 3.6 m diameters) were used. Asingle nozzle injected gas into the 76 mm column. Four nippleswere used as injection sites in the 1.8m diameter tank. Fifty-nineinjection sites (holes drilled in pipe wall) were used in the 7.6 mdiameter tank. H is liquid depth with no gas holdup and (kLa)20 ismass transfer coefficient at 20ºC in units of hr-1.

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Author Relation Basis2 Description

Khudenkoand Shpirt(1986)

kL a 0.041 h

db

0.67f

W

0.18U g

H

SE This relation was developed via dimensional analysis and calibrationwith experiments performed in rectangular tanks of three sizes.Liquid-gas systems were deoxygenated tap water and air. Twodiffusers and several diffuser spacings were employed. The transferparameter kLa has units of hr-1. Variables 1 and 2 are correctionsfor the presence of contaminants and the deviation of temperaturefrom 20ºC, respectively. H and h are the column height and aeratorsubmergence depth. W is the width of the aeration tank.

Roustan,Duguet et al.(1987)

kL a 0.0139U g0.82 E This expression was developed based on fitting an assumed power-

law relation between transfer rate and superficial gas velocity toexperimental data collected in a full-scale ozone contactor. The gas-liquid system observed was ozonated air – filtered water. Columnheight was 4.3 m and porous disc diffusers were used to introduceozonated air into the contactor. Units of kLa corresponding to thisrelation are min-1 and Ug is superficial gas velocity (gas volumetricflow rate divided by reactor cross sectional area) in units of m/hr.

Öztürk,Schumpe etal. (1987)

S h 0.62 S c0.5 Bo

0.33 Ga0.29 Fr

0.68 g

L

0.04 E Developed based on measurements in a cylindrical bubble column(diameter of 0.095 m, height of 0.85 m). A single gas distributorwas used with 50 different gas-liquid systems. Carrying gases wereair, nitrogen, carbon dioxide helium and hydrogen. Liquid phasewas 17 pure organic liquids and 22 mixtures of organic liquids withwater.

Uchida,Tsuyutani etal. (1989)

kL a dc2

Di

0.17 S c0.5 BO

0.62 G A0.31 g

1.1

0.17 D i0.5 dc

0.17 L0.12 g 0.93 L

0.62 0.62 g1.1

E Developed based on experimental measurement of oxygen transferinto deoxygenated liquids including distilled water, glycerolsolutions, butanol solutions and aqueous solutions containing asurface active agent. A right circular cylindrical bubble column wasoperated in countercurrent mode with variable superficial gasvelocities. A porous ball glass filter gas distributor and single nozzlewere used for air injection. Units for kLa are sec-1.

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8282

Author Relation Basis2 Description

Kawase andMoo-Young(1992)

kL

0.28g D i

2

L

1 3

Newtonian liquid, dB 2.5 mm

0.47g 2 D i

3

1 6

Newtonian liquid, dB > 2.5 mm

T Developed for rigid, small bubbles behaving as solid spheres andrising in Newtonian fluids. Trace amounts of contaminants maymake small bubbles behave as rigid spheres. Relations developed inthis study are similar to the empirical relations of (Calderbank andMoo-Young 1961) and provide theoretical backing for their use.The equations are dimensionally consistent. Relations are alsodeveloped for two-phase mass transfer in non-Newtonian liquids.

LeSauze,LaPlanche etal. (1993)

kL a U g

, 0.06, 0.5 Re 2100

0.06, 0.7 Re 2100

E Developed based on measurements in a pilot ozone contactor withcircular cross section, 4.3 m height, 0.15 m diameter, a porous platediffuser and undergoing countercurrent flow. Units of superficialgas velocity and kLa are m/s and s-1, respectively.

Roustan,Wang et al.(1996)

kL a 0.105U g

0.564 Re 680

0.055U g0.564 1912 Re 2986

E Developed for countercurrent flow of ozonated air bubbles in a pilotozone contactor (0.15 m diameter, 2.5m height) outfitted with aceramic porous distributor. The predominant bubble shape waselliptical. Units of kLa and Ug (superficial gas velocity) are min-1 andm/hr, respectively.

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II.1.2 Ozone Demand, Decomposition and Properties

When ozone is exposed to filtered water, there is a fast decrease in ozone

concentration followed by a decrease that can be modeled with first order kinetics

(Langlais et al., 1991; von Gunten 2003a). The stability of dissolved ozone is affected by

pH, ultraviolet light, ozone concentration and the concentration of ozone scavengers.

Because ozone decomposition kinetics are complex and because of the many factors that

influence the chemistry of ozone decomposition, rate constants are typically determined

experimentally for waters in batch experiments. Ozone decomposition is thought to be a

bimolecular process involving ozone and hydroxyl radicals and with a rate expression

given by:

d[O3]

d t k [O3][OH -] (22)

However, rate data are most often reported via a pseudo-first-order rate constant, kO3,

where

kO3

k

[OH -](23)

Researchers (LeSauze et al., 1993) have developed expressions of the form

log kO3 a b pH +c log[TOC] d log[TA] (24)

where a, b, c, and d are experimentally-determined constants and [TOC] and [TA] are

concentrations of total organic carbon and total alkalinity.

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Examples of rate constants and the conditions under which they were determined

are found in Table 13. Depending upon the water quality, ozone half-life in water can

range from the order of seconds to hours (von Gunten 2003a). Ozone decomposition is a

strong function of temperature, with ozone decomposing much slower at low

temperatures (below 10°C). Ozone plants operating in regions that undergo large

seasonal variations in raw water temperature must install ozone-quenching units

downstream of bubble contactors because low temperatures result in very high ozone

residuals downstream of ozone contactors presenting potential corrosion or human health

concerns. Conversely, high raw water temperatures necessitate application of high ozone

doses to maintain desired ozone concentration in contactors.

Table 13: Ozone Decomposition Rate Constants

kO3Source Conditions

0.011 s-1 Tang, Adu-Sarkodie etal. (2005)

Filter effluent from the ACWD treatmentplant, Fremont, CA, at 20°C, pH 7.3, 3.5mg/L TOC, total alkalinity 82 mg/L asCaCO3.

0.0025 s-1 Kim, Rennecker et al.(2002b)

Treated Ohio River water at 298 K (dataare given as activation energy andfrequency factor)

0.0017 - 0.018 s-1 Roustan, Wang et al.(1996)

Tap water (source not given) with 12ºC <T <19ºC, 7.5 < pH < 8.1, 75 < [TA] < 150mg/L and 0.8 < [TOC] < 6.0 mg/L

0.0045 – 0.019 s-1 Mariñas, Liang et al.(1993)

Filtered treated water with 12ºC < T <25ºCand 8.3 < pH < 8.4

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For mass transfer calculations, the most important ozone properties are ozone

Henry’s law constant and liquid phase molecular diffusivity. Ozone is considerably more

soluble in water than oxygen or nitrogen. Ozone’s Henry’s law constant increases with

temperature and pH and can be calculated using the expression:

KH 3.87107 [OH -]0.035 exp2428

T

(25)

where H is ozone Henry’s law constant in atm/L/mol and T is temperature in K (Langlais

et al., 1991). Molecular diffusivity also varies with temperature and can be calculated by

DO3 1.10106 exp

1896

T

(26)

where DO3has units of m2/s and T has units of K (Johnson and Davis 1996).

II.1.3 Disinfection Byproduct Formation

Von Gunten (2003b) divides ozone’s potential by-products into those formed in

the absence of bromide and those formed in the presence of bromide. Among those

formed in the absence of bromide, the predominant by-products are from the oxidation of

natural organic matter (NOM) by ozone. The resulting products can be aldehydes,

ketones, keto aldehydes, carboxylic acids, keto acids, hydroxy acids, alcohols and esters.

The main concern with these products is that they are readily biodegradable and may

promote biofouling in distribution systems. In the presence of bromide, disinfection

byproducts may include bromate, a regulated potential human carcinogen, and

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86

brominated compounds including trihalomethanes (THMs, presumed human carcinogens)

and halogenated acetic acids (HAAs, also regulated and among which are presumed

human carcinogens) (Westerhoff et al., 1998). The common ozone DBPs are illustrated

in Figure 13.

Figure 13: Significant Ozone Disinfection Byproducts (Song et al., 1997; UnitedStates Environmental Protection Agency 1999; von Gunten 2003b)

The most problematic ozone byproducts, are those formed in the presence of

bromine, and particularly bromate. Bromide occurs naturally in water due to salt-water

intrusion and special geological formations or due to human activity including coal

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mining, potassium mining and chemical production (von Gunten 2003b).

When ozone oxidizes NOM in the presence of bromide, a number of bromo-

organic byproducts may be formed. Concentrations of those compounds are usually far

below levels of human health concern. Bromate, however, has been classified as a

potential human carcinogen and the U.S. EPA has established a maximum contaminant

level (MCL) of 10 g/L for bromate in finished drinking water. In general, VonGunten

states that bromate production is not a concern for waters with a bromide concentration

less than 20g/L. For waters with bromide in the 40 – 100 g/L range, bromate

production may exceed acceptable levels and minimization strategies may have to be

employed. Above bromide concentrations of 100 g/L, bromate production during

ozonation will be very high.

Bromate forms in the presence of ozone via multiple pathways involving

dissolved ozone and hydroxyl radicals. Numerous authors (e.g., von Gunten (2003b))

indicate that both ozone and hydroxyl radicals must be included in a credible bromate

formation model and that “a simulation within a factor of two relative to the measured

bromate concentration has to be considered satisfactory” in modeling. An illustration of

the most significant pathways for bromate formation is shown in Figure 14. Note that the

mechanisms shown do not include NOM. In general, NOM tends to decrease bromate

formation by consuming bromide and ozone.

Roustan, Duguet et al. (1996) suggest that an approximate simplified bromate

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88

formation model is:

k1

O3 Br - BrO - O2 k1 160M -1s-1 at 20C

HOBr BrO - H pKa 9.0 (or 8.8) at 20C

k2

2 O3 BrO - 2O2 BrO3- k2 100M -1s -1 at 20C

Figure 14: Bromate Formation Pathways (Song et al., 1997)

Applying the Roustan bromate formation mechanism in ideal plug flow reactor (PFR)

and continuously stirred tank reactor (CSTR) models, the authors determined that at

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89

similar operating conditions the two reactor types discharged similar bromate ion

concentrations, but that to achieve a desired level of infection a CSTR requires a greater

Ct than a PFR. The authors caution strongly that the proposed bromate formation model

does not take into account hydroxyl radical formation and may yield misleading results.

Experimental investigations into the complex mechanism responsible for bromate

formation led Song, Donohoe et al. (1996) to the following conclusions:

increasing bromide, ozone dose, pH or inorganic carbon concentration increases

bromate formation;

Increasing dissolved organic carbon (DOC) or ammonia nitrogen tends to decrease

bromate formation;

Increasing contact time tends to increase bromate formation; and

increasing temperature tends to promote bromate formation.

The order of importance of the parameters in bromate formation is shown in Table 14.

Strategies for minimizing bromate formation in ozone contactors include

ammonia addition, pH reduction, hydroxyl radical scavenging or reduction of

hypobromous acid. The most practical of these solutions are ammonia addition and pH

depression (Pinkernell and Von Gunten 2001). In a study of concurrent inactivation and

bromate minimization, Driedger, Staub et al. (2001) demonstrated the feasibility of

bromate control while achieving target inactivation rates using both pH depression and

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ammonia addition.

Table 14: Factors Influencing Bromate Formation

Order of importance for parameters that tend to increase bromate formation:

pH > Ozone dose > Br - > Inorganic Carbon

Order of importance for parameters that tend to decrease bromate formation:

DOC > NH3-N

Absolute effect on bromate formation:

pH > Ozone dose > DOC > Br - < NH3-N Inorganic carbon

II.1.4 Microbial inactivation

Microorganisms respond differently to disinfectants and a number of models have

been developed to describe their inactivation rate. The models are based on general

behavior observed in disinfection experiments (“shoulders,” “tailing”) and an

understanding of the mechanisms by which disinfectants inactivate microorganisms. The

relations depend on kinematic parameters that are determined via statistical analysis of

experimental data collected in batch reactors. The most commonly used models,

corrected to account for first order disinfectant decay, are presented in Table 15 (Gyürék

and Finch 1998). In all the expressions in Table 15 except the Chick expression, the

degree of disinfection, Ct, includes changes in disinfectant concentration. In the Hom

and Hom power law expressions for batch survival, is the incomplete gamma function,

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defined as

(m, n k t) e z z m1dz0

n k t

(27)

Haas and Joffe (1998) proposed a method for developing inactivation relations for

use in continuous flow systems based on models developed for batch inactivation data.

Greene, Haas et al. (2001) demonstrated this procedure in their CFD simulation of

chlorine, chloramines and ozone disinfection of four microorganisms in a pilot scale

single-phase contactor.

Current practice and regulatory requirements assess reactor performance in terms

of “Ct” rather than by direct measurement of inactivation in water treatment. The Ct

approach acknowledges that the survival of organisms depends on the concentration of

disinfectant to which they are subjected (C) and the time over which they are subjected to

the disinfectant (t). Because ozone decays and is consumed during the disinfection

process, an average ozone concentration is used to calculate Ct. The contact time is

chosen conservatively as T10, the time for the first 10% of a conservative tracer to be

discharged from the reactor following the step introduction of the tracer to the reactor

inlet.

The Ct approach is practical given the difficulty of counting the myriad organisms

present in drinking water and given the time required to produce accurate counts, but

problematic given the variations encountered in disinfection process operations such as:

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variations in reactor hydraulics due to operation at off-design conditions;

variations in water quality leading to changes in disinfectant demand or microbial

sensitivity to the disinfectant;

influence of initial microbial density on inactivation rate; or

strain-to-strain variations in resistance to disinfection.

Table 15: Commonly-used Disinfection Models

Modelname

Predicted batch survival function

0

lnN

NKineticparameters Rate

Chick k C t k NCk

Chick-Watson

k C 0

n

n k*1 exp n k* t k, n NCk n

Hommk C 0

n

n k m m, n k t k, n, m m N k C n

1 m

lnN

N 0

11

m

Powerlaw

1

x 1ln 1

x 1 k C 0n

n k*N 0

x1 1 exp n k t

k, n, x xn NCk

Hompowerlaw

1

x 1ln 1 x 1

mk C on

n k* m m, n k t N 0

x1

k, n, m, x

m

m

n

xxxn

Ckx

NNNCkm

110

1

1

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Equally problematic is the tendency for the Ct approach, as it is currently

implemented for ozone contactors, to overestimate the required ozone dose or contact

time to achieve a given level of kill. Overestimating required ozone dose results in

excess costs and the potential for forming more disinfection byproducts than if a lower

ozone dose were used.

Ozone is the most potent chemical biocide studied by the U.S. EPA to date (Clark

and Boutin 2001). A summary of inactivation data generated by several researchers for

ozone disinfection is presented in Table 16. Giardia muris and Cryptosporidium parvum

exhibit a temperature dependent lag phase when exposed to ozone (von Gunten 2003b).

Table 16: Summary of Ozone Inactivation Data (Clark and Boutin 2001)

Organism

Ct

L

minmg LogReduction Conditions

Indigenous aerobicbacterial endospores

19 3 Filtered Ohio River water attemperatures between 23.6 and 25.2ºC

Polio virus 1.2 2 Filtered Ohio River water attemperatures between 23.6 and 25.2ºCand pH 7.6

Giardia muris 1.9 2 Unknown water source, temperature of5ºC and pH of 7

Giardia lamblia 0.55 2 Unknown water source, temperature of5ºC and pH of 7

Giardia muris 0.75 2 Filtered Ohio River water, temperaturebetween 23 and 24C and pH 7.65

Cryptosporidiumparvum

5 2 Conditions not described

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Organism

Ct

L

minmg LogReduction Conditions

Cryptosporidiumparvum

6.56 2.5 Temperature of 25ºC, other conditionsnot described

Cryptosporidiumparvum

4 1.4 Filtered Ohio River water, temperaturebetween 23 and 24C and pH 7.65

The action of ozone on pathogenic organisms has been debated, with the debate

fueled by a wide variation in published values for rate constants of organisms of interest

in water treatment. In one camp are those who believe that direct action of ozone on

microorganisms is the dominant mechanisms of inactivation. In the second, indirect

action of ozone through generation of hydroxyl radicals is assumed to be the dominant

mechanism in inactivation. Based on comparison of inactivation rates in the presence of

dissolved ozone with inactivation rates for organisms exposed to known concentration of

hydroxyl radicals, von Gunten (2003b) states that the predominant mechanism for

inactivation is direct action of ozone, with hydroxyl radicals playing a minor role.

II.2 Experimental Investigations of Bubble Column Reactors

The many published experimental investigations of phenomena in bubble column

reactors can be grouped into:

mass transfer investigations and

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95

hydrodynamics investigations.

II.2.1 Experimental Measurement of Mass Transfer in Bubble Columns

To date, bubble column mass transfer investigations have involved measurement

of dissolved gas concentration at discrete locations along the bubble column reactor.

Experiments are performed for a range of gas and liquid flow rates and, in some cases,

with different water qualities.

LeSauze (1993) performed tracer studies and estimated ozone mass transfer for a

4.2 m tall, 0.l5 m diameter bubble column. Ozone mass transfer rate estimates were

based on analysis of samples drawn from sample ports located at the reactor top and

bottom and three intermediate depths. The precise depths of the intermediate sample

ports are not provided. Tracer and ozone mass transfer experiments were conducted at

three superficial liquid flow rates (0.86, 1.42, and 1.97 cm/s), four superficial gas flow

rates (0.076, 0.087, 0.203 and 0.48 m/s) and for influent gas-phase ozone concentration

ranging from 0.463 to 2.142 g/m3). Rather than use ozone residual data for developing a

rate expression for ozone mass transfer, the authors used an empirical relation for ozone

mass transfer from a prior study and assessed several combinations of ideal reactor

models to determine the one which best fit measured ozone residual data. Based on their

results, the authors suggested the following criteria be used in design of ozone contactors:

for water disinfection, reactors approaching plug flow conditions yield continuous

residual and optimal performance;

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for use of ozone in oxidation of dissolved matter, reactors hydraulics should approach

complete mixed performance;

for realistic reactors which must achieve both objectives, reactors should be designed

in tow stages: a completely-mixed stage whose effluent is the ozone residual required

for disinfection followed by a plug flow stage that facilitates contact between

disinfectant and microorganisms.

To ascertain the influence of water quality on ozone mass transfer and

disinfection performance, Owens (2000) measured the influent ozone concentration,

effluent ozone concentration and ozone concentration for samples drawn from 4 equally-

spaced intermediate ports in an ozone bubble column of 0.15 m diameter and 2.65 m

height. The contactor was operated in countercurrent mode at a liquid flow rate of 6.4

L/min and a gas flow rate of 0.64 L/min. Ozone mass transfer rate was not estimated

directly in this study; rather, CT values corresponding to the depths of each of the

intermediate ports were determined by numerical integration of measured residual ozone

concentrations and assuming liquid flow rate equal to superficial velocity. Bromate

concentration was also measured in samples drawn from the influent, effluent and

intermediate ports. The authors concluded that, for Ohio River water, there is a trade-off

between the log removal of Cryptosporidium parvum oocysts and production of bromate.

In a study which compared ozone and peroxone (water with dissolved ozone gas

and hydrogen peroxide) for pre-oxidation to improve filter performance (Tobiason et al.,

1992), ozone dissolved into raw water in a 3.05 m tall, 30.5 cm diameter bubble column

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97

run in countercurrent mode. Net ozone mass transfer was estimated based on gas phase

measurements of ozone in the feed gas and off-gas. Experiments were performed at a

liquid flow rate of 37.8 lpm and a gas flow rate of 16.5 slpm and at ozone doses ranging

from 0 to 0.75 mg/L. No ozone mass transfer analyses were performed in this study.

Both ozone and PEROXONE were found to extend filter runs when used in combination

with coagulant doses typically used in treatment at the New Haven, CT drinking water

treatment plant.

In another pilot study investigating the difference between ozone and

PEROXONE, Scott (Scott et al., 1992) dissolved ozone into pilot plant filter effluent in

four 5.2 m tall, 15.4 cm diameter cylindrical bubble columns arranged in series. Contact

time (taken to be equal to the effluent ozone residual multiplied by T50) was varied

between 2.16 and 5.23 mg-min/L). As in other pilot studies, ozone mass transfer rate was

not directly calculated. Ozone residual in the effluent was seen to vary “unpredictably”

with given dose. The authors did not speculate as to the cause of these variations, though

they advised use of measured residual rather than applied dose for estimating disinfection

in ozone contactors. The variation seen in ozone residual has been observed in full scale

contactors (Schulz and Bellamy 2000) and is likely related to hydrodynamics and sample

acquisition.

II.2.2 High-Resolution Study of Bubble Column Hydrodynamics

Several experimental techniques have been employed for observation and

quantification of hydrodynamics in bubble columns. Though techniques are available for

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98

observation of bubble motion in an ensemble of bubbles, these techniques have most

often been applied for measurement of liquid-phase motion. These techniques provide no

direct measurement of mass transfer rate or dissolved gas concentration.

Particle image velocimetry (PIV) consists of laser sheeting, image recording and

data processing (Chen and Fan 1992). Images can record the position of bubbles in the

plane of the laser sheet and, when the liquid phase is seeded with visible particles, the

position of the particles suspended in the liquid phase (Degaleesan et al., 2001). In image

processing, procedures must be developed for distinguishing individual bubbles and

particles and for tracking particles and bubbles from frame to frame. Because the liquid

phase is usually seeded with visible particles, this technique has, to date, only been used

in bubble columns with non-flowing liquid phase. Versions of PIV have been used to

measure spatial variations in gas hold-up in a bubble column with non-flowing liquid

phase (Delnoij et al., 1999), to measure spatial variations in gas hold-up and turbulence

intensity in a two-phase system (Liu et al., 2005) and to make general observations of

flow in a three-phase system with non-flowing liquid and solid phases (Chen and Fan

1992). PIV allows visualization of features that influence countercurrent mass transfer

(back-mixing and non-uniform hold-up) but does not allow direct measurement of the

effects of these phenomena on mass transfer.

Another experimental technique for quantifying hydrodynamics in bubble

columns is the computer-automated radioactive particle tracking (CARPT) procedure. In

contrast to PIV, CARPT experiments do not visualize flow on a single plane in the

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99

bubble column. Rather, the positions of individual radioactive particles are tracked (in

three dimensions) as they are carried by the liquid phase. The advantage of this

technique over PIV is that it provides information on hydrodynamics in the entire reactor.

CARPT has been used to investigate the flow field (presence of circulation and

distribution of turbulence intensity) in bubble column reactors with non-flowing liquid

phase (Degaleesan et al., 2001).

II.3 Ozone Contactor Modeling

II.3.1 CFD Models

Four researchers have published papers on CFD ozone bubble columns modeling

studies. These studies are described below and summarized in Table 17.

In a study performed for the Metropolitan Water District of Southern California,

Henry and Freeman (1995) developed a finite element model of a full-scale ozone

contactor. The commercial code FIDAP (formerly licensed by Fluid Dynamics Inc.,

currently by Fluent Inc.) was used to perform a two-dimensional, two-phase simulation of

a proposed full-scale contactor. Bubbles were assumed to have fixed diameters of 3 mm

and were modeled via a Lagrangian approach. Details on gas boundary conditions are

not provided.

The CFD model was used to simulate a tracer study and results were compared

with experimental data. The authors report an average deviation of CFD study tracer E

curve values (expectation) of 6.8% from experimental values. The E curve (also called

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100

the exit age or residence time distribution curve) is a plot of measured or predicted tracer

concentration as a function of time and normalized by intake tracer concentration. Plotted

experimental and computational tracer curves indicate the CFD model significantly over-

predicts dispersion. Having modeled tracer studies, the authors modeled potential design

modifications to the ozone contactor including:

Alternate water depth to contactor length ratios;

Alternate baffle gap spacing to chamber length ratios;

Addition of vanes, corner fillets and wall foils.

Sketches showing the baffle gap, vanes, fillets and wall foils are provided in Figure 15.

In general, greater water depths and wider baffle spacing gaps result in higher

T10:HDT. T10 is the time at which 10% of the tracer exits the contactor and HDT is the

contactor hydraulic detention time. Higher T10:HDT indicates more uniform contacting

of water with dissolved ozone and is generally desirable. Addition of vertical vanes in

the contactor (to direct flow passing through baffle gaps) had a pronounced effect on

RTD, increasing predicted T10:HDT by 8%. Fillets provided only minor improvement in

hydraulic performance. Adding wall foils produced a 4.8% increase in predicted

T10:HDT.

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101

Figure 15: Ozone Contactor Design Modifications (Henry and Freeman 1995)

A progenitor to the commercial CFD code CFX was used to assess design

modifications to a full-scale ozone contactor employed at the Alton Water Treatment

Works, Anglian Water, UK (Murrer et al., 1995). The authors performed the study in the

hopes of developing an alternative to expensive, time consuming and complicated

experimental studies. A schematic diagram showing the contactor is found in Figure 16.

Few details of the CFD model are provided in the published results. The model

was three-dimensional and two-phase, though details on treatment of multiphase

momentum and mass transfer are not provided. The authors state that the model was

calibrated via modifications and comparison with pulse tracer studies, though it is unclear

what they take calibration to mean and what model parameters may have been adjusted.

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102

Excellent correlation of simulated and experimental tracer curves is claimed without

reference to any quantitative measure of correlation.

Following successful calibration of the CFD model, the authors extended the

model to include ozone transfer between phases and ozone demand in the aqueous phase.

A bench-scale experimental study was performed to ascertain bubble size, rise rate and

growth rate. Employing these data, CFD simulations were able to predict ozone residual

in the full scale reactor accurately. Finally, the authors predicted the reactor performance

under varied operating conditions, with modified diffuser placement and with additional

baffling in the final chamber of the contactor. The CFD model predicted significant

improvement in reactor performance when the gas flow rate in the first bubble contacting

chamber (see Figure 16) was higher than in the second and when a baffle was added to

the last chamber in the reactor.

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103

Figure 16: Murrer, Gunstead et al. (1995) Reactor Schematic

Cockx, Do-Quang et al. (1999) performed the most inclusive CFD study of an

ozone contactor to date. In the study, CFD was used to simulate two-phase flow, ozone

mass transfer and ozone decomposition in a full-scale bubble contactor. The contactor

modeled was comprised of seven chambers whose combined volume is 350 m3 and with

a capacity of 53,000 m3/day. A schematic diagram of the contactor is presented in Figure

17.

The authors used the finite volume CFD code ASTRID for analyses. An

Eulerian-Eulerian treatment of two-phase flow was employed with provisions made for

momentum and mass transfer between the phases. Momentum exchange between the

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phases is calculated as

ML ap

1

2lCDVr Vr (28)

where ML is the mean volumetric momentum transfer to the liquid phase from the gas

phase for a control volume, ap is projected volumetric interfacial area (L2 projected

surface area per L3 reactor volume), l is liquid phase density, CD is drag coefficient

(described below) and Vr is the relative speed between the phases (the slip velocity). The

authors assumed ellipsoidal bubbles with attendant volumetric interfacial area of

ap 3

2

g

b(29)

where g is local volumetric gas fraction and b is the projected bubble diameter on a

horizontal plane. Without explanation, the authors selected a drag coefficient of 1.0.

Bubble diameter was assumed uniform and constant and equal to 3 mm. No mention is

made of bubble-induced turbulence (Sato and Sekoguchi 1975) and it is assumed the

authors did not account for that phenomenon.

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Figure 17: Reactor Schematic for Cockx CFD Study

Mass transfer of ozone between the gas and aqueous phases, given as

Ll kLa (CL* CL ) (30)

where Ll is mean volumetric mass transfer to the liquid phase, kL is the interphase

transfer coefficient, a is volumetric interfacial area (L2 bubble surface area per L3 reactor

volume), CL* is the saturation concentration of ozone corresponding to the gas-phase

ozone partial pressure and CL is mean local aqueous ozone concentration. Without

providing insights into the reasons for their choice, the authors use the Higbie (Motarjemi

and Jameson 1978) relation for mass transfer coefficient:

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106

a 6 g

db

; kL 2DO3

Vb

db

(31)

where DL is molecular diffusion (L2/T) for dissolved ozone in water. Direct use of the

Higbie relation is questionable, since it was developed for large bubbles with mobile

surfaces in pure water. The influent water is assigned an instantaneous ozone demand of

0.24 mg/l and aqueous phase ozone decay is assumed to follow first order kinetics with a

rate constant of 0.12 min-1.

Cockx compared results from the resulting CFD model with experimental tracer

study data and particle image velocimetry (PIV) data collected in a pilot study. The pilot

study data are not reported. RTD curves for experimental and simulated tracer studies

appear to agree well, through no statistical or quantitative measure of their agreement is

presented. Based on apparent success in simulating tracer experiments, the authors

simulated a modified reactor in which baffles were added to the chamber to inhibit short-

circuiting and promote slug flow. In CFD simulations of the modified reactor, Ct

(presumably at the reactor discharge) was increased 165%. In experiments (whose

details are not described) Ct was improved 114%.

In the most recent published ozone contactor CFD study, Huang, Brouckaert et al.

(2002) developed a model for a full-scale ozone contacting system. The ozone contactor

modeled in that study is a retrofit of a chamber whose primary use is water disinfection.

The contactor is located at the Wiggins Water Works, Durban, South Africa. It consists

of a static mixer, located immediately upstream of the contactor, in which ozonated air is

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107

injected into the water stream and all ozone is assumed dissolved into the aqueous phase.

No data are presented to support the assumption that all ozone is transferred from the gas

phase prior to introduction of the water/gas mixture into the contact chamber. Ozonated

water is introduced into the contact chamber via an inlet located in the chamber bottom.

The contact chamber is of serpentine design and water exits the contactor via a weir.

Huang used the commercial CFD code FLUENT for numerical analyses and used

FLUENT’s preprocessor, GAMBIT, for developing a mesh. A - turbulence model was

employed and the presence of bubbles was approximated via augmented turbulence

intensity of the inlet stream. Only heuristic justification was provided for approximating

the gas phase in this manner. Inlet turbulence intensity was adjusted to provide the best

match between computational and experimental tracer studies. The inlet (located on the

contactor floor) was modeled as a Dirichlet boundary condition. The free surface was

approximated as a horizontal rigid lid. The outlet weir was approximated as a submerged

rectangular slot and a frictional loss coefficient was assigned to the weir to account for

head loss over the weir.

Experimental tracer studies were performed for the contactor with and without

gas injection. The presence of injected gas made a relatively minor difference in the

shape of the tracer curves. Computational tracer studies were performed and turbulence

intensity, defined as

IT

2

3

V(32)

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108

was varied. In equation 1, IT is turbulence intensity (dimensionless), is turbulent

kinetic energy (L2/T2) and V is mean fluid speed (L/T).

The authors found that an inlet turbulence intensity ratio of 50% provided a better

match between experimental and computational tracer curves than an inlet turbulence

intensity ratio of 20%. This conclusion was based on qualitative comparison of

experimental and simulated tracer curves. The authors state that the good agreement

between simulated and experimental tracer studies validate their model and justify the

simplifications employed, especially their simplified treatment of two-phase flow.

Table 17: Summary of Ozone Contactor CFD Studies

Author Code andformulation

Two-phasemodel

Turbulencemodel

Masstransfermodel

Ozonechemistry

Inactivationmodel

(Henry andFreeman1995)

FIDAP/FE Eulerian-Lagrangian

- None None None

(Murrer et al.,1995)

CFX/FV Eulerian-Eulerian

Unknown Unknown Demand None

(Cockx et al.,1999) and(Do-Quang etal., 1999)

ASTRID/FV

Eulerian-Eulerian

- Higbie Instanta-neousdemand,1st-orderdecay

Chick

(Huang et al.,2002)

FLUENT5.5.14/FV

Modifiedinfluentturbulenceintensity

- None None None

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II.3.2 Other Models

Ozone contactor modeling has historically been performed using one-dimensional

axial dispersion models or tanks in series models. These models have provided insights

into gross design principles and have provided a means for analyzing data collected in

laboratory and pilot scale plants but do not have an obvious role in detailed investigation

of bubble column phenomena or design of full scale contactors. Several ozone contactor

models are described below, with emphasis on their successes and limitations.

LeSauze, LaPlanche et al. (1993) modeled countercurrent ozone mass transfer in a

bubble column using three ideal reactor models and a fourth model in which portions of

the reactor were modeled via different models. The ideal reactor models employed were

a completely stirred tank reactor (CSTR) model, a plug flow reactor (PFR) model and an

axial dispersion model. In the hybrid model the portion of the reactor near the sparger

was modeled via an axial dispersion model with high dispersion, the middle portion of

the reactor was modeled as a PFR and the top portion of the reactor was modeled via an

axial dispersion model with a moderate level of dispersion. The hybrid model results

provided the best match with data collected in an experimental bubble column.

Zhou and Smith (1994) developed an axial dispersion model of a countercurrent

ozone bubble contactor and used the model to predict the performance of a bubble

contactor for varying liquid and gas flow rates and feed gas ozone concentrations. Mass

transfer coefficients were estimated via the Deckwer correlation (Table 12) and

corrections were made for aqueous phase ozone decay. The authors made a limited

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number of comparisons of model outputs with experimental data and described the data

that would be required to perform more rigorous validation of the model.

Finally, Kim, Tomiak et al. (2002a) developed an axial dispersion model inclusive

of ozone mass transfer, ozone demand, ozone decay and microbial inactivation. The

resulting ordinary differential equations are presented below. Numerous assumptions

were made in development of this modeling, including first-order ozone decay, second

order reaction of ozone and natural organic matter (NOM), uniform steady bubble

diameter, uniform axial dispersion in the bubble column and Chick-Watson inactivation

kinetics (with n=1).

0

0

0

0

,2

21

,2

21

,,2

21

3

LNae

NOMLNOMaNOMNOM

e

L

H

gSH

g

NOMLNOMaLOaL

H

g

SLL

e

CNDzd

Nd

zd

NdP

CCDzd

Cd

zd

CdP

CK

C

S

N

zd

K

Cd

CCDCDCK

CN

zd

Cd

zd

CdP

(33)

In these expressions, z height above the column bottom, CL and Cg are liquid and gas

phase ozone concentrations, Da,I is Damkhöler number for the reaction in which species i

is consumed, N is number of microorganisms per unit volume, NS is Stanton number and

S is a stripping factor, defined as

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111

L

g

U

UmS (34)

Auxiliary relations for bubble diameter, mass transfer coefficient, Henry’s law

constant and microbial inactivation rate were used to determine constants found in the

above equations and the resulting equations were solved simultaneously.

The authors compared predicted ozone transfer and microbial inactivation to

experimental data with generally favorable results. The authors cautioned strongly

against general application of this model to other contactors without careful examination

of parameter estimations. Application of this model to a full-scale reactor with three-

dimensional flow patterns would be problematic. Specifically, several assumptions used

in developing the axial dispersion model are invalid for the hydraulically-complex flows

encountered in full-scale reactors. Questionable or invalid assumptions include uniform

dispersion, uniform gas phase distribution in the reactor, and one-dimensional transport

within the reactor.

II.4 Other Bubble Contactor CFD Studies

As recounted below, researchers have applied numerous techniques in developing

CFD models for bubble contactors. In this section the major modeling choices for CFD

simulation of bubble columns are presented and examples of studies using various types

of models are described. The majority of the bubble contactor papers identified in the

literature were analyses of bubble columns in which gas was bubbled through stagnant

liquids and the authors were interested mainly in hydrodynamics, not mass transfer.

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Several authors noted the lack of bubble column experimental data in the open literature

for comparison with CFD simulations (Mitra-Majumdar et al., 1998; Sanyal et al., 1999).

The same can be said for axially-resolved and radially-resolved mass transfer data. Thus,

in the short term validation of modeling approaches and exploration of submodels will be

a major hurdle for researchers simulating bubble columns with CFD.

In simulating a bubble column via CFD, the major choices that must be made are:

Treatment of two-phases (Eulerian-Eulerian, Lagrangian-Eulerian, Algebraic Mixture

Model or Direct Numerical Simulation);

Choice of steady or transient simulation;

Choice of domain (2-dimensional or 3-dimensional);

Turbulence model (-, -, large eddy simulation [LES] or perhaps others); and

Choice of submodels for interphase momentum transfer and mass transfer (perhaps

accounting for interactions of bubbles with each other), bubble size (perhaps

accounting for coalescence) and turbulent dispersion enhancement due to bubbles.

Among the numerous papers in the literature describing CFD simulation of bubble

contactors, several are reviewed below to illustrate these different approaches.

Ranade (1997) undertook CFD studies of bubble columns because, like Mitra-

Majumdar et al., he felt one-dimensional approaches lack generality (are applicable only

for designs and operating conditions for which experimentally-derived constants are

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valid). Studies were performed for air-water systems with bubbles whose diameter

varied from 3 mm to 8 mm. The objective of the work was to reproduce numerically the

tendency of bubbles to migrate toward the center of a cylindrical bubble column in

heterogeneous bubble flow. To account for this, the author resorted to an artificial, if

effective, device – the imposition of the following condition on bubble drag:

FD a br

R

1 2

(35)

In the above relation FD is the drag force on the bubble at radial coordinate r, R is the

bubble column radius and a and b are constants equal to 2.2 and 1.7, respectively. The

constants a and b were chosen to reproduce observed distribution of the gas phase in the

reactor and are believed to account for bubble-bubble interactions. The ratio of bubble

drag coefficient to diameter was chosen to be 290 m-1. Not surprisingly, the author

achieved good qualitative agreement with experimental values. The agreement was

assessed via graphical comparison of axial mean velocity and turbulence intensity and

radial gas phase holdup.

In a demonstration that CFD can be applied to increasingly complex bubble

column flows, Mitra-Majumdar, Farouk et al. (1998) developed a CFD model of two and

three-phase co-current flow of water, air bubbles and glass beads. An Eulerian-Eulerian

treatment of the multiple phases was used and both the gas and solid phases were treated

as dispersed phases. Both experiments and CFD simulations were performed and radial

and axial gas and solid phase holdups were compared with experimental data. In general,

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the two-phase CFD model predicted radial variation in gas phase holdup well, while the

three-phase model did not fare as well, perhaps due to the choice of drag model in the

three phase CFD simulations.

Pfleger, Gomes et al. (1999) performed CFD and experimental investigations of a

bubble column with stagnant water and air bubbles sparged into a rectangular channel.

The position of the sparger and gas flow rate were varied and two-dimensional and three-

dimensional transient simulations were performed. The commercial CFD code CFX 4.2

was used for the CFD simulations and the two-phase system was modeled as Eulerian-

Eulerian. Time steps were 0.01 seconds and the total simulated (real) time was 400

seconds. A fixed bubble diameter and drag coefficient were specified.

The authors noted a marked difference between two-dimensional and three-

dimensional simulations, with the three-dimensional calculations far better estimating

experimentally measured turbulence intensity and qualitative behavior (transient drift) of

the bubble plume in the column. The authors determined that the keys to performing a

tractable and realistic bubble column simulation were to use three dimensions and a fine

length scale. The - turbulence model employed for the liquid phase appeared adequate

for producing realistic results.

Eulerian-Eulerian and Algebraic slip mixture model two phase flow treatments

were compared directly in a study performed by Sanyal, Vásquez et al (1999). The

authors used the commercial CFD code FLUENT (Fluent, Inc., Lebanon, N.H., USA) to

perform transient, two-dimensional simulations of a circular cylindrical bubble column in

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which air was sparged into stagnant water. A single bubble diameter was chosen to

represent the bubble size distribution and bubble drag was calculated via a relation for a

single sphere dropping in an infinite fluid (the precise relation is not provided in the

paper). Time steps were 0.01 seconds for Eulerian-Eulerian simulations and 0.005

seconds for simulations using an algebraic slip mixture model two-phase treatment. The

turbulence model was - and a uniform grid (0.66 cm axial 0.5 cm radial)

approximated the geometry.

The authors found good agreement between results generated using both two-

phase models when bubbly flow was simulated but found significant difference when

churn turbulent flow was simulated (no mention is made of changes in bubble diameter or

coalescence for heterogeneous bubble flow). Both models tended to over predict the

centerline axial velocity. Though the authors did not draw this conclusion, this result is

consistent with the experience of Pfleger et al. (1999) and indicates that two-dimensional

bubble column simulations have limitations. However, Sanyal concluded that two-

dimensional axisymmetric models provide “good engineering descriptions” of bubble

column hydrodynamics and holdup. The authors indicated the need for better turbulence

modeling and prediction of turbulent diffusivity.

In a CFD simulation of a bubble plume in a cylindrical column whose diameter is

much greater than the plume diameter, Bernard, Maier et al. (2000) used a single-phase

flow code, MAC3D (Army Corps of Engineers Waterways Experiment Station,

Vicksburg, MS, USA) with source terms added to the momentum equation to simulate

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vertically-rising bubbles. The authors dub this approach the drift-flux model. The

advantages of this approach are obvious – single-phase calculations are much easier to

perform and require less computational effort than multiphase codes. MAC3D is a finite

volume code and a - turbulence model was employed for the liquid phase. Walls were

modeled as no-slip boundaries and the free surface was approximated as a rigid lid.

Bubbles were assumed to have a uniform diameter and plume geometry was imposed on

the solution. The model reproduced steady velocities in the bubble plume within a factor

of two and the authors believe the far-field mixing effects of a bubble plume in a

reservoir were well characterized. The authors indicated their intent to perform future in

which the model accounts for stratified liquids.

Large Eddy Simulation (LES) and - models were compared for Eulerian-

Eulerian simulation of bubble column flow by Deen, Solberg et al. (2001). Results from

CFD simulations were compared to experimental data and the two turbulence models

were compared. The bubble column in that study was a rectangular cross-sectioned

cylinder outfitted with a distributor plate with 49 holes of 1 mm diameter. Grid spacings

for the - turbulence model simulations were 101010 mm. Coarse (101010 mm)

and fine (4.7104.7 mm) grid spacings were used in LES simulations. Transient flow

was modeled and time steps of 0.01 sec and 0.005 seconds were used for the - and LES

simulations, respectively. Bubble diameter was uniform and steady and set equal to 4

mm. The drag coefficient was chosen to be 1.0 based on the computed value of Eötvös

number. The Sato model for enhanced turbulence (Sato and Sekoguchi 1975) was

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employed.

Comparison of profiles of simulated and experimental liquid axial velocity

profiles, axial gas velocity profiles, radial liquid velocity fluctuations and turbulent

kinetic energy profiles showed clearly that the LES turbulence model produced better

agreement between calculations and experiment. LES computations took 90 hours to

complete on a 4-processor, high-end workstation. No data are provided on the

computational requirements for the - simulations.

The Euler-Lagrange approach to two-phase modeling in a bubble column was

employed by Laín, Bröder et al. (2002). A comparison of the Eulerian-Eulerian and

Eulerian-Lagrangian approaches summarized from that paper is presented in Table 18.

Table 18: Comparison of Eulerian-Eulerian and Eulerian-Lagrangian Approaches

Approach Eulerian-Eulerian Eulerian-Lagrangian

Liquid phase Navier-Stokes equations withsource terms added for bubblemomentum transfer

Navier-Stokes like equationscoupled with Navier-Stokes likeequation for gas phase

Gas phase Newtonian equations of motionwith bubble-bubble interactionsvia collision models

Navier-Stokes like equationscoupled with Navier-Stokes likeequations for liquid phase

Appropriateapplications

Dilute two-phase flows andheterogeneous bubbly flows.

Dense flows. Validity isquestionable for very dilute flows(Laín et al., 2002)

Advantages Accounts for a spectrum of bubblesizes and allows modeling ofbubble break-up and coalescence

Computational efficiency. May beused to predict bubble coalescenceif bubbles are represented bymultiple dispersed phases (Olmoset al., 2003)

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CFD simulations and experimental results were compared for a bubble column

(air-water) with stagnant water and a membrane aerator. Based upon previous

experience, the authors used a distribution of bubble diameters (the precise distribution is

not stated) and calculated drag coefficient as:

CD

16Re1 Re 1.5

14.9Re0.78 1.5Re 80

48Re1 1 2.21Re

0.5 1.861015 Re4.756 80 Re 1500

2.61 Re 1500

(36)

where Re is Reynolds number based on the bubble diameter and magnitude of the

velocity difference between the bubble and liquid. Transient, two-dimensional

calculations were performed.

Time-averaged mean and fluctuating velocity profiles (axial and radial) were

compared with experimental values and good agreement was claimed. In general, the

authors determined that accurate modeling of bubble column flow with the Eulerian-

Lagrangian approach requires:

Inclusion of relevant bubble class sizes in the Lagrangian model;

Use of an appropriate relation for drag coefficient that distinguished between

Reynolds number regimes; and

Application of appropriate source terms in a - turbulence model to account for

interphase momentum transfer.

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III EXPERIMENTAL METHODS

Two types of laboratory experiments were performed in a bubble column

operated with countercurrent flow:

Residence time distribution (RTD) studies and

Ozone mass transfer visualization studies.

RTD studies generated data that allowed evaluation of column hydrodynamics

and characterization of mixing. These data were used to relate mixing intensity to

column operating conditions and in validation of the proposed CFD model. Ozone mass

transfer visualization studies enabled quantification of spatial variations in mass transfer

in the reactor and were also used in CFD model validation.

As described in the literature survey, numerous experimental methods for

investigation of hydraulics and mass transfer in bubble column reactors have been

employed in prior studies. None of these methods were deemed appropriate for

generating data about mass transfer at the fidelity desired in the current study.

For example, in all prior ozone bubble column mass transfer studies (Scott et al.,

1992; Tobiason et al., 1992; Mariñas et al., 1993; Owens et al., 1994; Saberi et al., 1995;

Owens et al., 2000; Kim et al., 2002a; Kim et al., 2002b; Charlton 2003) ozone mass

transfer rate was estimated based on discrete measurements of ozone residuals at the

bottom and top of the reactor or at six or fewer intermediate positions along the reactor.

These measurements allowed mass transfer rate estimates, but were not sufficiently

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resolved to relate mass transfer to hydrodynamics and did not result in expressions for

mass transfer that could be scaled. Other experimental studies such as those employing

phase-Doppler anemometry (PAD) (Laín et al., 1999), particle image velocimetry (PIV)

(Chen and Fan 1992; Delnoij et al., 1999; Liu et al., 2005) or computer-automated

radioactive particle tracking (CARPT) (Chen et al., 1999; Degaleesan et al., 2001)

provided highly-resolved data on distribution of bubbles or flow field, but did not yield

information about mass transfer. Additionally, since the PIV and CARPT techniques

require seed of particles in the liquid phase, they are generally performed for bubble

columns with non-flowing liquid phase.

Because the techniques outlined above could not provide mass transfer data at the

resolution desired, a novel technique for obtaining mass transfer data was developed.

This technique is described in detail in III.3. The only prior study that employed a

similar technique (image analysis of images taken of flow in a countercurrent flow

bubble column reactor) (Rice and Littlefield 1987; Baird and Rao 1998) investigated

dispersion, not mass transfer.

III.1 Experimental Apparatus

Experiments were performed in the 15.2 cm diameter, 1.83 m tall glass bubble

column reactor shown in Figure 18 and depicted schematically in Figure 19 and Figure

20. As reported in the literature review of this dissertation, all pilot and laboratory

continuous flow bubble column ozone contactors studies found in the literature employed

circular cylindrical reactors (Roustan et al., 1987; Scott et al., 1992; Tobiason et al.,

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1992; LeSauze et al., 1993; Mariñas et al., 1993; Kim et al., 2002a; Kim et al., 2002b;

Charlton 2003). The reactors used in these prior studies differed only in their inlet and

outlet configurations, diffuser type and location, and operating conditions. The reactor

chosen for the current study was selected because it was similar to reactors used in prior

pilot studies of ozonation in bubble columns (allowing easy comparison of performance

with reactors used in prior studies) and because a suitable column was available for use at

Drexel following relatively minor modifications.

Figure 18: Experimental Reactor Photograph

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The column’s liquid feed is a mixture of tap water and stock solution. For tracer

studies the stock was a dilute solution of sodium chloride. In ozone visualization

experiments the stock solution was a 100% dilution of potassium indigo trisulfonate dye

reagent (described below). The tap water stream was metered via a rotameter and the

stock solution stream was delivered by a metering peristaltic pump (Fisher Scientific

[provide model number]). A 30 cm in-line helical static mixer mixes the two liquid

streams approximately 60 cm upstream of the introduction of the liquid stream into the

reactor. The liquid stream is introduced to the reactor through two ports (0.64 cm

diameter) in the bottom of the reactor collar. The collar was packed with 7 mm beads

that dissipate the inlet liquid stream momentum and promote uniform flow into the

bubble column. Liquid flows downward in the bubble column, exiting the reactor via

four symmetric discharge ports in the bottom of the reactor. The bottom of the reactor is

packed with 7 mm glass beads to promote uniform flow and reduce the impact of

discharge design on flow in the reactor.

Gas flows into the reactor via a 2.5 cm spherical fine bubble diffuser located

approximately 5 cm above the reactor bottom, as depicted in Figure 21. In tracer

experiments the gas feed is compressed air and in ozone mass transfer visualization

experiments the gas feed is ozonated compressed air. A rotameter measures gas flow

feed rate. Off gas is vented from the top of the reactor. For experiments in which

ozonated air is bubbled in the reactor, the off-gas is bubbled in a closed flask under a

chemical fume hood (to allow measurement of off-gas ozone concentration). Discharge

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from the closed flask is then fed to a solution of sodium thiosulfate to ensure destruction

of residual ozone.

Bubblecolumn

To drain

In-linemixer

Ozonedestruction

Dischargegas phase

ozonemeasurement

Stocksolution

Liquid flow path

Gas flow path

Rotameter

Tapwater

Gas feed

Gas discharge

123.4

Liquid feed

Liquid discharge

Spherical diffuser

Intake collar

Figure 19: Laboratory Bubble Column Schematic Diagram (not to scale)

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Figure 20: Reactor Schematic Diagram, Scale Drawing

Figure 21: Scale Drawing of Laboratory Column Bottom

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125

III.2 Residence Time Distribution Studies

Step tracer experiments were used to generate data for residence time distribution

analyses. Stock solutions of sodium chloride tracer were mixed to provide a tracer

concentration of 500 mg/L in the reactor liquid feed. This concentration was chosen

because it provides a sufficient variation in liquid feed conductivity for accurate

measurement of tracer breakthrough but does not have a large enough difference in

density from that of tap water to influence hydrodynamics (Bartrand et al., 2005). Salt

concentration was measured as conductivity with a VWR dip cell conductivity meter

(model 2052). A plot showing conductivity measured by the conductivity probe as a

function of salt concentration is presented in Figure 22. Because conductivity is a linear

function of sodium chloride concentration over the concentration range used in tracer

experiments, conductivity measurements were used instead of salt concentrations in

residence time analyses.

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CNaCl (g/100 mL)

0 1 2 3 4 5

Con

duct

ivit

y(m

S)

0

10

20

30

40

50

60

70

Figure 22: Conductivity Probe Calibration

Prior to step tracer experiments, the liquid stock was tap water and the reactor was

operated at steady gas and liquid flows for at least 4 theoretical hydraulic residence times.

At the beginning of tracer experiments (time = 0 sec) the liquid stock solution was

changed from tap water to sodium chloride solution. Samples were taken from the liquid

discharge line approximately 8 cm downstream of the reactor discharge at 15 second

intervals. After approximately 4 theoretical hydraulic residence times, the stock solution

was switched to tap water and samples were taken for an additional 4 theoretical

hydraulic residence times. Both step-up and step-down experiments were performed so

that effects of tracer density on the tracer curve might be identified. A typical tracer

curve is shown in Figure 23.

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127

0.0

0.2

0.4

0.6

0.8

1.0

0.0 1.0 2.0 3.0 4.0 5.0 6.0 7.0 8.0 9.0

t /

F

Figure 23: Typical Tracer Curve

In Figure 23, as in subsequent analyses, tracer data are normalized and presented as an

“F” curve, where

backgroundfeed

backgroundtracer

CC

CCF

(37)

and time is non-dimensionalized by theoretical hydraulic residence time, tH. In equation

35, Ctracer is the conductivity immediately downstream of the reactor discharge, Cfeed is

the conductivity at the reactor intake and Cbackground is the background (tap water)

conductivity.

Residence time distribution data (F, ) were fit to the five residence time

distribution models depicted in Figure 24. The single stream N-CSTR and 1-dimensional

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128

ADR (advection dispersion reaction) models (Figure 24(a) and Figure 24 (c)) were

chosen because of their widespread use in reactor analysis (e.g., LeSauze et al., 1993;

e.g., Kim et al., 2002a). Parallel stream models (Figure 24(b) and Figure 24 (d)) were

chosen to account for the presence of two streams in two-phase flow – one associated

with downward flow of liquid outside the bubble plume and a second associated with

downward flow of liquid within the bubble plume. The cell backflow model (Figure

24(e)) was chosen because entrainment of liquid into the bubble plume was observed

during flow visualization and because of reported successes modeling two phase flow

with the cell backflow model (Nauman and Buffham 1983; El-Din and Smith 2001(b)).

a. N-CSTRmodel

b. ParallelN-CSTRs

c. 1-D ADRmodel

d. Parallel1-D ADRs

e. Cellbackflowmodel

Q

qQ + q

Q Q

x Q (1 – x) Qx Q (1 – x) Q

QQ

Figure 24: RTD Model Schematic Diagrams

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129

It can be shown that the residence time distribution of a step tracer for an N-

CSTR reactor model is given by the equation (Haas et al., 1997):

Dt

t

DttE

H

H

H

H

4

1

exp

2

1

2

(38)

where D is dispersion, H is mean hydraulic residence time, and t is time. This

distribution depends upon two parameters, D and H. Rather than reporting dispersion

directly, mixing is usually reported via the dimensionless parameter Peclet number,

defined as

D

LUP L

e (39)

where UL is liquid superficial velocity (volumetric flow rate divided by reactor cross

sectional area), and L is characteristic length (reactor height for bubble column reactors).

The inverse Gaussian function provides an approximation for the residence time

distribution for the axial dispersion model. This distribution is a function of two

parameters, mean hydraulic residence time and variance of the inverse Gaussian

distribution, , and an approximation to the distribution is given by (Haas et al., 1997):

t

t

ttE

2exp

2

2

3(40)

The parallel stream models are linear combinations of equations 38 and 40 of the

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130

form

tEtEtE 21 1 (41)

where is an additional parameter that provides the distribution of mass flow in the

parallel reactors. The parallel reactor distributions are functions of 5 parameters.

Although approximations to the cell backflow model have been proposed in the

literature (Retallick 1965) they are accurate over small ranges in the number of cells and

the amount of backflow between cells (q) and use of the full model equations for

modeling two phase flow is recommended (Nauman and Buffham 1983). Consequently,

best fit model parameters for the cell backflow model were determined by comparing

numerical solutions of the cell backflow model equations to experimental measurements.

III.3 Ozone Mass Transfer Visualization Studies

III.3.1 Overview

The objective of ozone mass transfer visualization experiments was to establish

steady flow conditions and obtain a digital photograph showing the distribution of a

reactive dye in a reactor.

Ozone mass transfer studies proceeded as follows:

1. Air was sparged into the reactor at a steady rate and off-gas from the head space was

vented through tubing and bubbled in water from a Milli-Q water system (Millipore

Intertech, Bedford, MA).

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2. A mixture of reactive dye (buffered solution of potassium indigo trisulfonate) and tap

water was introduced to the reactor at a steady rate.

3. As dye filled the reactor, samples were taken from the reactor discharge at two

minute intervals. Dye concentration was determined from these samples via a

spectrophotometric measurement at 500 nm in a Barnstead/Thermoline

Spectrophotometer, model 340.

4. After at least 4 theoretical hydraulic residence times, steady conditions were assumed

to exist and the dye concentration was assumed uniform. While the reactor was being

filled with dye solution, water samples were taken from a sample port approximately

8 cm downstream of the reactor discharge at 2 minute intervals. After the completion

of experiments, the dye concentration in the samples was measured and used to

confirm that steady conditions had been achieved.

5. The ozone generator (shown in Figure 19) was switched on at a chosen voltage. The

voltage was chosen to ensure that enough ozone was supplied to the column to ensure

a significant difference in dye color between the top and the bottom of the column,

but not so much ozone that all the dye was decolored prior to discharge from the

column.

6. The liquid feed rate, gas feed rate and ozone generator voltage were held steady for at

least three reactor theoretical hydraulic residence times, during which time the ozone

decolored the dye and a quasi-steady distribution of dye was established in the

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reactor. The dye distribution was quasi-steady (rather than steady) because

turbulence in the reactor liquid flow caused fluctuating dye concentrations throughout

the reactor.

7. During the dye decoloration process, digital photographs were taken of the reactor at

2 minute intervals (details of the photographic setup are provided below) and samples

were withdrawn from the sample port downstream of the reactor discharge at 2

minute intervals. The digital photographs were used for calculating ozone mass

transfer rate and the samples were used to verify that quasi-steady conditions had

been established.

8. The liquid discharge temperature was noted and the water feed, gas feed and ozone

generator were turned off.

9. The ozone concentration in the water through which the off-gas was bubbled was

determined using the indigo trisulfonate method (American Public Health Association

1998).

10. The reactor was refilled with tap water and digital images of the reactor (with no dye

or bubbles) were taken. These images were used to remove variations in background

lighting from the images taken of indigo dye at quasi-steady distribution.

Important components of these steps are described in detail below.

III.3.2 Indigo Dye Solution Composition and Preparation

The dye used in ozone mass transfer visualization experiments is a buffered

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133

solution of indigo potassium trisulfonate. Indigo trisulfonate is shown in Figure 25. In

solution, the carbon double bond of indigo trisulfonate reacts rapidly and preferentially

with ozone, decoloring the molecule (Bader and Hoigné 1981). One mole of ozone is

consumed per mole of indigo trisulfonate decolored. To determine whether tap water

contained constituents that interfered with the ozone-indigo dye reaction the indigo dye

method was used to measure the ozone concentration in a samples diluted with milli-Q

water and tap water. Ozonated air was bubbled into mill-Q water for 15 minutes (until a

steady ozone concentration was established) and 20 mL samples were transferred to 4

flasks containing 10 mL of indigo dye reagent. Two of the flasks were filled to 100 mL

with milli-Q water and two were filled to 100 mL with tap water. Absorbance at 500 nm

was determined via spectrophotometer. Experiments were conducted at 3 ozone residual

concentrations. In all cases there was no difference between absorbance (and ozone

concentration) between the samples diluted with tap water and those diluted with milli-Q

water. This indicated that tap water consitutents did not interfere with the ozone-indigo

reaction and that no treatment of tap water was necessary prior to use in ozone mass

transfer visualization experiments.

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134

Figure 25: Indigo Trisulfonate Structure and Daughter Products

Prior to performing ozone mass transfer visualization experiments, test runs were

performed in which indigo dye was fed to the reactor at known concentrations and flow

rates and the ozone generator was operated at a range of voltages. These test experiments

identified a range of indigo dye concentrations and ozone generator voltages that

produced significant dye without causing complete decoloration anywhere in the reactor.

decoloring was observed but the discharge water was not completely decolored.

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III.3.3 Photography Methodology

The setup for recording digital images was developed to

Provide uniform lighting of the reactor;

Provide images that spanned as much of the reactor as possible while still providing

high resolution;

Ensure photographs taken in different experiments were taken under the same

conditions.

Backlighting was used to provide uniform illumination of the reactor. The

lighting setup is shown in Figure 26.

The light sources were two high-temperature fluorescent lamps, 2.44 m (8 ft) tall,

mounted on the frame holding the bubble column. Because the lamps extended above

and below the reactor, variations in lighting along the reactor length were relatively

minor. The greatest variations in lighting occurred at the reactor top and bottom, where

light was partially blocked by the horizontal PVC sheets supporting the column. The

camera (Nikon Coolpix 8700, Nikon Corporation, Tokyo, Japan) was positioned 1.68 m

(66 in) from the front of the reactor. This position was chosen to maximize the reactor

height visible with zero zoom.

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136

Figure 26: Mass Transfer Visualization Experiment Lighting

III.3.4 Development of Indigo Dye Color Calibration Curve

Prior to performing the steps outlined above, the relationship between the color

recorded in digital images and the indigo dye concentration was established. This

relationship was established by

filling the reactor with solutions of indigo reagent diluted with tap water,

taking samples and digital photographs of the reactor filled with dye,

plotting the dye concentration against the absorbance of the dye (measured via

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137

spectrophotometer at 500 nm),

processing digital images to account for variations in background lighting and

plotting mean color of digital images against indigo dye concentration.

Experiments were performed at 6 indigo trisulfonate concentrations. The highest

concentration was chosen to be higher than any concentration that would be encountered

during ozone mass transfer visualization experiments.

Image processing consisted of:

Subtracting an image of the reactor filled with a known dye concentration from an

image of the reactor filled with tap water (the background).

Inverting the color of the resulting image.

Cropping the image to include only the reactor.

Removing the glass manufacturer’s mark by “cloning” an area immediately above the

mark over the black lettering.

Converting the image from 32-bit RGB JPEG image to an 8-bit (grey scale) TIF

(tagged image file) format.

Determining the mean pixel value and mode pixel value for the 8-bit image.

Image processing was performed using the public domain image processing software

ImageJ, version 1.34s (Rasband 2005). Processed digital images showing the dye color

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138

at 6 dilutions are presented in Figure 27.

(a) 0.64 mg/L (b) 1.28 mg/L (c) 2.57 mg/L (e) 5.13 mg/L (f) 6.42 mg/L(d) 3.85 mg/L

Figure 27: Pixel Color Calibration Images

Histograms showing distribution of pixel color for the images shown above are

shown in Figure 28. The abscissas of the plots in Figure 28 are the pixel color (in 8-bit

grayscale). A pixel value of 0 indicates a completely black pixel and a pixel value of

256 indicates a completely white pixel. The histograms exhibit sharp peaks at distinctly

different pixel values over the range of indigo dyes examined. These sharp peaks at

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139

distinct colors indicate that pixel color is a reliable indicator of indigo dye concentration.

Calibration of indigo dye concentration with pixel color is described below.

0.64 mg/L 1.28 mg/L0.64 mg/L0.64 mg/L 1.28 mg/L1.28 mg/L

2.57 mg/L 3.85 mg/L2.57 mg/L2.57 mg/L 3.85 mg/L3.85 mg/L

5.13 mg/L 6.42 mg/L5.13 mg/L5.13 mg/L 6.42 mg/L6.42 mg/L

7.70 mg/L7.70 mg/L

Figure 28: Calibration Image Histograms

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A plot of absorbance at 600 nm versus indigo trisulfonate concentration for

dilution of indigo reagent in tap water is presented in Figure 29. The linear dependence

of absorption on indigo trisulfonate concentration indicates that:

The constituents of tap water do not significantly alter the absorbance of solutions of

indigo trisulfonate at 600 nm, and

Absorbance at 600 nm is a linear function of indigo trisulfonate concentration.

0

1

2

3

4

5

6

7

8

9

0 0.1 0.2 0.3 0.4 0.5 0.6

Indigo trisulfonate concentration (mg/L)

Ab

sorb

an

ce

Data

Least Squares Fit

Figure 29: Variation of Absorbance with Indigo Concentration for Indigo ReagentDiluted with Tap Water

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141

Plots showing pixel value mean and mode for the images shown in Figure 27 and

Figure 28 versus known indigo dye concentration are presented in Figure 30. Curves

were plotted for images with and without the background subtracted and for the mode

and mean of the pixel values. Note that images are 8 bit gray scale. As such, pixel color

ranges from 0 to 256, with 256 corresponding to white (0 indigo dye concentration) and 0

corresponding to black. The curves corresponding to images with the background

subtracted are offset from those in which the background was not subtracted. This

indicates that the subtraction of the background pixel color does not affect the final image

color (monochromatic blue in RGB channels). Two important observations can be made

based on Figure 30:

For all curves, the variation in mean and mode of the pixel color is linear with indigo

dye concentration and

over the concentration range expected to span the concentrations during experiments,

there is a significant change in pixel color intensity.

These observations indicate that the pixel color intensity is a sensitive indicator of

indigo dye concentration and that a calibration curve relating pixel intensity to indigo dye

concentration may be developed. The calibration curve based on mean pixel color with

the background subtracted and is shown as a solid line in Figure 30.

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142

0

50

100

150

200

250

300

0 1 2 3 4 5 6 7

Indigo Trisulfonate Concentration (mg/L)

Pix

elC

olo

r(8

bit

;0

=B

lack

,2

56

=W

hit

e)

Pixel color mean, background subtracted

Pixel color mode, background subtracted

Pixel color mean, background not subtracted

Pixel color mode, background not subtracted

Calibration curve

r2 = 0.985

Figure 30: Pixel Color Calibration Curve

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143

IV NUMERICAL METHODS

IV.1 Mathematical Model

A two-phase model (Eulerian-Eulerian) is employed for the numerical solution of

the gas/liquid flowfields and phase distributions. In this model, the phases are modeled

as uniformly mixed within a given mesh element and the volume occupied by phase in

that mesh element is denoted . In the current two phase study, L is liquid volume

fraction, G is gas volume fraction and G + L = 1.0.

Assuming no source terms for the liquid and gas phases and no mass transfer

between phases due to phase change, the two-phase model continuity and momentum

equations are:

0

V

t

(42)

and

FVVPVVV

t

T (43)

where , V, P and are the density, velocity, pressure and viscosity of phase ,

respectively, and F is the interfacial force acting on phase due to the presence of the

other phase. For the current problem, the only interfacial forces of significance are drag

force and interphase turbulent dispersion force and

TD FFF

(44)

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144

where DF

is the interfacial force due to drag and TF

is interfacial force due to turbulent

dispersion.

The drag component of the interfacial force term is given as

VVAC

F DD

8

(45)

where CD is drag coefficient, A is the net interfacial area between the phases and V

and

V

are the velocities of phases and . The Grace relation was chosen for drag

coefficient because bubbles were observed to be elliptical and dispersed. The Grace

drag coefficient (Clift et al., 1978) is:

LT

B

DU

dgC

23

4(46)

where g is gravitational acceleration, dB is mean bubble diameter, is the difference in

density between the phases, L is liquid phase density and UT is bubble terminal rise

velocity, given by

857.0149.0 Kd

UBL

LT

(47)

In the terminal velocity expression, is the Morton number (a fluid property) given by

32

4

L

L g (48)

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145

where is surface tension and K is given by

3.5942.3

3.59294.0441.0

751.0

BB

BBK (49)

In equation 20, B is given by

14.0

149.0

3

4

ref

LEoB

(50)

and Eo is the Eötvös number, given by

2

bdg

Eo

(51)

Turbulent dispersion force is given by

L

L

G

G

Lt

Lt

dTD

T CCF

,

,

(52)

where CTD is an empirical constant (taken to be 1.0 in the absence of data for turbulent

dispersion force in countercurrent flow), Cd is drag coefficient (described above), t,L is

turbulent viscosity, t,L is liquid turbulent Schmidt number (taken to be 0.9) and G and

L are the gas and liquid phase volume fractions, respectively.

The two equation turbulence model (-) for the continuous (liquid) phase is

LLtLL

k

Lt

LLLLLLL PkUt

,

,

(53)

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146

2,

,

LLtL

Lt

LLLL PUt

(54)

In equations 46 and 47, is the turbulent kinetic energy, is the characteristic turbulence

frequency, t,L is the liquid phase turbulent viscosity and the constants , ', k, and

are 0.075, 0.09, 2, 2 and 5/9, respectively. The liquid phase turbulent viscosity is

modeled using the Sato particle enhanced turbulence model (Sato and Sekoguchi 1975),

given in equation 48:

ptstLt ,,, (55)

where t,s is the conventional shear-induced turbulent viscosity and t,p is a particle

induced component of turbulent viscosity given by

LGbgLppt UUdC

,, (56)

and C,p is given a value of 0.6. The term Pt,L in equations 46 and 47 is the turbulence

production due to viscous forces, calculated as

LtT

tLt UUUUUP

33

2, (57)

The dispersed (gas) phase turbulence is modelled using a zero equation model in

which gas turbulent viscosity is proportional to liquid phase turbulent viscosity:

gt

Lt

L

GGt

,

,

,

(58)

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147

where t,g is a turbulent Prandtl number relating the dispersed phase kinematic eddy

viscosity to the continuous phase kinematic eddy viscosity. In calculations, t,g was

assumed to equal 1, the standard value used in the absence of detailed turbulent kinetic

energy measurements.

The governing equation for transport of a conservative scalar quantity (tracer) in

the continuous (liquid) phase is given as

T

T

T

LTLLTLTL CSc

DUCCt

,

(59)

where CT is volumetric concentration of the tracer, DT,L is diffusivity of the tracer in the

liquid phase and ScT is turbulent Schmidt number. Because there is no mass transfer of

the tracer to the dispersed phase, there is no scalar transport equation for the dispersed

phase.

Dirichlet inlet boundaries were specified for water (at the top) and air (at the

bottom). A degassing boundary condition for the gas (no slip for the liquid phase, sink

term for the gas phase) was specified at the top of the reactor. In the laboratory reactor

the top of the reactor is a free surface and gas leaves the water at the free surface and

flows through a sealed plenum and escapes the plenum at a port located in the center of

the plenum top. Four pressure boundaries, located in the bottom of the column, make up

the water discharge boundary. In the laboratory reactor, the region between the sparger

and water discharge is packed with 7 mm glass beads. This volume is simulated in CFD

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148

as a porous volume with transmissivity of 0.01 cm2. The transmissivity was estimated

using the Karman-Cozeny relation.

Simulations were started as steady state and results from steady simulations were

used as initial conditions for transient simulations. It was found that the following initial

conditions yielded a relatively fast (within 500 iterations) convergence to an rms (root

mean square) residual of 1×10-4 for all variables:

Uniform gas velocity equal to the predicted single bubble terminal rise velocity;

Uniform downward liquid velocity equal to the water volumetric flow rate divided by

the reactor cross sectional area.

Small gas volume fraction, uniform throughout the reactor.

IV.2 Numerical Model

The governing equations described in the earlier sections were solved numerically

for specified initial and boundary conditions with the commercial finite volume CFD

package CFX (ANSYS Europe Ltd. 2004) on a 3-dimensional unstructured mesh. Mesh

density was chosen based on a grid resolution study and generated to provide high

resolution at column walls and near the diffuser.

To assess the grid resolution, gas volume fraction along the column diameter

shown in Figure 31 was calculated at three mesh densities (coarse, medium and fine). In

grid resolution studies, steady flow was assumed, the gas phase was monodisperse with a

mean bubble diameter of 2.5 mm and a - turbulence model was employed. As

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149

described below, steady flow is reasonable to assume when the bubble column is

perfectly vertical. When a slight lean (< 0.5º from vertical) is included, the bubble plume

is not steady in the center of the column and a transient simulation is required.

The coarse, medium and fine density grids had 140,000, 372,000 and 712,000

tetrahedral elements, respectively. In grid resolution studies the gas and liquid flow rates

were 2 L/min and 6.6 L/min. Results from the grid resolution study are presented in

Figure 32.

Because differences in the gas fraction profile were minor between the medium

and fine meshes, the mesh used in the present study is a refinement of the medium

density mesh. Prism elements were added to the medium mesh at the column walls and

the grid was refined locally in the vicinity of the sparger, water intake and the top of the

column (where water enters the column from the intake section). The resulting grid has a

total of 470,000 tetrahedral and prismatic elements.

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150

Figure 31: Diameter Along which Grid Resolution Study was Performed

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151

Figure 32: Gas Volume Fraction Profiles

A second-order upwind transient scheme with relatively small time steps (0.05 s)

was required to achieve convergence to an RMS residual of 1×10-5 within 10 iterations

per time step. To produce representative “quasi-steady” results, calculations were

performed for approximately 10s of simulation time, after which variations in bubble

plume shape became minor and bubble plume was seen to rotate in the column, though

not with a fixed period.

IV.3 Model Validation

Based on the observations of Rice and Littlefield (1987) and observations in the

laboratory, it was noted that minor misalignments of the column (of less than 0.5° off

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152

vertical) or its components (e.g., sparger locations) can drastically change gas and liquid

flow and mixing. Despite efforts at leveling the column, locating the diffuser in the

column center and ensuring even flow through inlet and discharge ports, it was surmised

that perfect alignment of the column was unlikely. So the CFD model included a slight

(0.25°) vertical tilt. In the absence of this tilt, CFD predicted a perfectly symmetric

bubble plume. When the tilt was included the plume exhibited the asymmetric plume rise

observed in bubble column experiments. Specifically, the plume tended to migrate

toward the column wall and spiral as it ascended.

The countercurrent flow model was validated using tracer data (described below).

In the CFD model, a non-reactive, conservative tracer was introduced as a step feed in the

liquid phase at time 0s and the concentration of the tracer at the reactor discharge was

calculated at regular time intervals. The CFD model reactor discharge is shown in Figure

21. This study is referred to as a “virtual tracer study.”

Gas flow rate and liquid flow rate for the virtual tracer study were 2 L/min and

6.6 L/min, respectively. A plot showing normalized experimental tracer concentration

(F) and virtual tracer normalized concentration versus normalized time (t / tH) is

presented in Figure 33. The virtual tracer curve shown in Figure 33 is a plot of

instantaneous tracer concentration, area-averaged at the reactor discharge. The definition

of normalized tracer concentration is given in equation 37 (repeated below).

BackgroundFeed

BackgroundTracxer

CC

CCF

(37)

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153

The CFD model reproduced measured residence time distribution data reasonably

well, predicting a slightly earlier breakthrough than that experimentally observed and

matching experimental data more closely at later times. In Figure 33, the CFD model

(the solid line) shows greater variation than the experimental data (symbols). This is

because the CFD model was “sampled” at 1 second intervals and via a point

measurement, whereas the experimental tracer studies used samples taken at 15 second

intervals and requiring approximately five seconds to draw. The agreement between

observed and predicted RTDs is considered excellent given the complexity of the flow

and the use of a two-equation turbulence model.

0

0.05

0.1

0.15

0.2

0.25

0.3

0.35

0.4

0 0.1 0.2 0.3 0.4 0.5 0.6 0.7

t / t H

F

Numerical

Experimental

Figure 33: CFD Model Validation

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154

V COUNTERCURRENT FLOW HYDRODYNAMICS INVESTIGATIONS

Experimental and numerical studies performed are summarized in Table 19. As

described above, tracer studies entailed introduction of a step input of sodium chloride

tracer at the reactor inlet and monitoring the conductivity of water at the reactor

discharge. Conductivity is a linear function of salt concentration over the concentration

range used in these studies. Tracer studies generated data for calculation of Peclet

number and characterizing dispersion. Tracer studies were performed at a single liquid

flow rate (6.6 L/min) and a range of gas flow rates chosen to span the ideal bubbly flow

regime.

Table 19: Countercurrent Flow Hydrodynamics Experimental and NumericalStudies

Study Liquid flow rate(s)(L/min)

Gas Flow Rate(s)(L/min)

FlowVisualization

6.6, 10.5, 13.5 0.4, 0.7

ExperimentalTracer

6.6 0, 0.5, 1.0, 1.5, 2.0,2.2, 2.4, 3.0, 3.5

CFD Studies 6.6, 13.5 0.4, 1.0, 1.5, 2.0, 2.5

In flow visualization studies, rather than a salt tracer, a non-reactive dye was

introduced to the reactor as a step function. Flow visualization studies were performed at

two gas flow rates (0.4 and 0.7 L/min) and liquid flow rates of 6.6, 9.0 and 12.0 L/min.

Flow visualization studies showed phenomena related to early breakthrough of tracer.

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155

V.1 Bubble Plume Behavior and Flow Visualization

As gas flow rate was increased, the behavior of the bubble plume changed

significantly, though no increases in bubble break-up or collisions were observed. At a

low gas flow rate (0.5 L/min) and a liquid flow rate of 6.6 L/min, the plume rises

vertically and increases in diameter with height, as shown in Figure 34(a). Analysis of

high-resolution digital images indicates bubbles range in shape from nearly spherical to

oblate and bubbles tend to ascend in a spiral or zigzag path. At a higher gas flow rate

(2.5 L/min), the bubble plume rotates while rising, tending to migrate away from the

column centreline and toward the wall as shown in Figure 34(b). At some distance above

the sparger (typically between 0.6 and 1 m), the plume expands to fill the entire column.

b) High gas flowrate

a) Low gas flowrate

Figure 34: Photographs of Bubble Plume Shapes

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156

Flow visualization at a water flow rate of 6.6 L/min and a gas flow rate of 2.0

L/min is shown in Figure 3. The individual frames show the progress of the dye at 30 s,

1 min, 1 min 30 s and 2min after the start of dye injection. Digital image processing was

used to remove variations in image color caused by uneven illumination. The black mark

seen at approximately one third the reactor’s height is the glass manufacturer’s mark.

As with salt tracer studies, in flow visualization studies the reactor was operated

at steady state for 4 theoretical hydraulic residence times prior to the introduction of the

non-reactive dye (dilute solution of buffered sodium indigo trisulfonate) to the reactor.

The dye was fed at a steady rate and concentration for 4 theoretical hydraulic residence

times. The color (darkness) of the image is proportional to the concentration of the dye.

The linear relationship between image color and dye concentration was ascertained

through analysis of digital images of the reactor filled with uniform solution of dye at 7

dilutions as described in section 0.

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157

(a) 30 s (b) 1 min (c) 1 min 30 s (d) 2 min

Figure 35: Flow Visualization – Dye Progress at 30s, 1 min, 1 min 30s and 2 min(the Dark Triangle Approximately 1/3 the Reactor Height in Each Image is the

Glass Maker’s Manufacturer’s Mark)

The liquid phase does not exhibit plug flow behavior; dye proceeds unevenly in

the column, tending to flow faster near the column wall. Preferential flow of the dye near

the column wall is seen in frames (a) – (c). As the dye plume proceeds down the column,

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158

dye is entrained into the bubble plume (in the center of the column) and back-mixes with

the down-flowing stream. This is seen in Figure 35(d). In that frame the front of the dye

plume is better mixed than in the prior 3 frames. Based on these observations, one can

expect early tracer breakthrough (due to the rapid progress of the dye near the column

wall), and a long tail on the residence time distribution arising from back-mixing of the

tracer into the bubble plume.

V.2 Residence Time Distribution Analysis

Experimental “F” curves corresponding to a liquid flow rate of 6.6 L/min and gas

flow rates ranging from 0 to 3 L/min are presented in Figure 36. The parameters and F

are the normalized time (t / tH) and the normalized concentration, defined above in

equation 37.

The early portions of the F curves in Figure 36 indicate that increased gas flow

rates promote earlier breakthrough. This is due, in part, to upward flow of liquid phase in

the bubble plume (“gulfstreaming”) and reduction of the effective column cross sectional

area through which downward-flowing liquid passes. Because the late portions of the F

curves approach the value 1.0 very slowly, it is clear there is significant hold-back or

back-mixing of the tracer in the reactor. This is likely due to entrainment of the tracer

into the bubble plume and transport of the tracer upward in the reactor.

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159

0.0

0.2

0.4

0.6

0.8

1.0

0.0 0.5 1.0 1.5 2.0

F

No gas flow

Q = 0.5 lpm

Q = 1 lpm

Q = 2 lpm

Q = 3 lpm

Earlybreakthrough

Figure 36: Experimental Residence Time Distributions (RTDs) for 0 < Qg < 3 L/min

As described above, nonlinear regression was used to fit candidate residence time

distribution models to the experimentally measured residence distribution curves. The

gamma function (an approximation to the solution of the transient N-CSTRs in series

model) and the inverse Gaussian function (an approximation to the solution of the axial

dispersion model) were fit to the data by varying their model parameters. Since both

models have two parameters, the best fit model was the model yielding the lowest sum of

squares of errors between the model prediction and the experimental data. For all gas

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160

flow rates the inverse Gaussian model provided the best fit to experimental data.

Peclet number, in environmental engineering applications, is defined in equation 53

(repeated below) (Weber 2001)

L

Ltcee

E

HUSRP ,

where Re is Reynolds number, Sc,t is turbulent Schmidt number, UL is liquid phase

superficial velocity, H is reactor height and EL is turbulent dispersion. Peclet number was

calculated from the variance of the inverse Gaussian distribution fitted to the tracer data

using equation 4 (repeated below)

eP

eeePP 122 21 (60)

where v is the dimensionless variance ratio.

Experimental relations found in the literature for Peclet number in countercurrent

bubble columns are presented in Table 20. With the exception of that of Baird and Rice,

all the relations presented in Table 20 were developed based residence time distribution

analysis of tracer. Baird and Rice developed their relation using analysis of images

captured on video cassette. In their work, they followed the mixing of two solutions of

different pH by tracking the front of a pH sensitive dye.

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161

Table 20: Countercurrent Flow Peclet Number Relations

Relation Study

b

cg

Lv

duE

2

Bischoff and Phillips (1966)a

23.0 0.3G b c

e

L

u v dP

E

Reith et al. (1968)b

1 3 4 30.35

Ge

G C

u HP

u g d

Baird and Rice (1975)c

7 61 2

1

5 3

4.880.00185 9.7 G L

e

L b

uP

H u d

(Kim et al., 2002a)d

a Based on analysis of data from numerous small diameter cocorruent, countercurrent and nonflowingliquid phase bubble columns. Only valid in the ideal bubbly flow regime.b Based on experimental data taken in 5 cm and 14 cm cocurrent and countercurrent bubble columns inwhich air was sparged into tap water. The term 2ug + vb is the relative velocity between phases.c Developed using dispersion data collected from several studies and under the assumption of isotropicturbulence and turbulent energy dissipation rate equal to (ug g).d Developed for co- and countercurrent flow in a 15 cm circular bubble column. Units of H is in m and allother units must be dimensionally consistent.

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162

0.1

1.0

10.0

100.0

1000.0

0 0.5 1 1.5 2 2.5 3 3.5 4

Gas Flow Rate (L/min)

Pec

let

Nu

mb

er

Reith

Kim

Baird

Experimental

CFD

Figure 37: Experimental and Predicted Peclet Number

Figure 37 shows Peclet number calculated from experimental data (as described

above) plotted along with Peclet number estimates from relations for countercurrent

bubble column Peclet number found in the literature and with estimates made using CFD

calculations. The experimental estimates of Peclet number are shown with a 90%

confidence interval. To estimate Peclet number from CFD calculations, the volume

averaged specific turbulence energy dissipation rate, , was calculated for each gas flow

rate and used in the expression proposed by Baird and Rice (1975) to calculate axial

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163

dispersion

313435.0 cL dE (62)

The corresponding Peclet number was calculated using equation 53. Note that although

the parameter EL is usually called “axially dispersion” in environmental and chemical

engineering literature, the dispersion in the reactor is not uniform in the axial direction

and the term EL would be more aptly referred to as the average turbulent dispersion.

Peclet number falls sharply as gas flow increases from 0 to 0.5 L/min, is relatively

constant (around 3.0) for moderate gas flow rate and falls as gas flow rate increases

above 2 L/min. The Kim expression (listed in Table 20) fits experimental data well at

low and high gas flow rates. Reith estimate (listed in Table 20) fits the data at moderate

gas flow rate. Baird and Rice’s approximation to equation 31 ( cG dU ) consistently

underpredicts Peclet number.

CFD estimates for Peclet number offer the best match to experimental data,

falling within a 90% confidence interval around experimental values at intermediate gas

flow rates. Like experimental values, CFD estimate of Peclet number does not vary

significantly at intermediate gas flow rates. This agreement indicates that the CFD model

accounts for the important hydrodynamics in this regime.

Summarizing experimental observations, RTD analyses indicate three flow regimes

encountered over the range of gas flows. At low gas flow rate (1 L/min and below) there

is very little backmixing and the Peclet number falls sharply with increasing gas flow

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rate. At intermediate gas flow rates (1.5 L/min ≤ Qgas≤ 2.5 L/min), the Peclet number is

relatively constant. In this regime the bubble plume rises asymmetrically in the column

and rotates as a function of time near the sparger. At high gas flow rates Peclet number

falls slightly and backmixing increases significantly. Churn turbulent behaviour

(significant bubble break-up and coalescence) was not observed during any experiment.

V.3 Numerical Studies

Numerical studies were performed to develop a detailed understanding of the

mixing phenomena and trends identified in experimental studies. Specifically, details

were sought on the variation in mixing over the axial extent of the reactor. Transient

simulations, summarized in Table 19, were performed at a liquid flow rate of 6.6 L/min

and gas flow rates ranging from 0.4 to 2.0 L/min. These cases were used to estimate

Peclet number (shown in Figure 37) and to generate velocity vector diagrams for

exploration of the changes in flowfield that occur with increasing gas flow rate.

A “virtual tracer study” was also performed in which the step feed and passage of

a conservative tracer through the reactor was simulated. Gas and liquid flow rates for the

virtual tracer study were 2.0 L/min and 6.6 L/min, respectively. Figure 38 shows

contours of virtual tracer concentration at 20, 40 and 60 s after introduction of the tracer.

Red indicates the tracer concentration is equal to the feed concentration and blue

indicates zero tracer concentration. The images in Figure 38 compare favorably with the

experimental flow visualization images found in Figure 35. As seen in experiments, the

CFD model predicts that the tracer projects downward into the reactor along the reactor

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sides, swirling as it progresses.

Figure 38: Virtual Tracer Concentration at 20s, 40s and 60s after Step Input

Contours of gas volume fraction, g, predicted at a gas flow rate of 2 L/min are

shown in Figure 39(a). The plume does not rise symmetrically, but migrates in the

column and finally migrates to the wall near the top of the column. The plume region,

shown in Figure 39 (b) is defined as the region within which the liquid phase velocity is

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upward. The surface shown in Figure 39 (b) is an isosurface where liquid vertical

velocity, wL, is equal to zero. Note that there is upflow of liquid in the bubble plume over

the entire reactor height and that the plume twists as it rises in the column. These figures

illustrate non-axisymmetric plume rise and significantly different plume shape near the

sparger compared with higher locations. In drinking water treatment, non-asymmetric

flow as illustrated in Figure 39 creates the potential for short-circuiting of raw water and

retards ozone mass transfer via poor mixing in the bubble plume and reduced contact of

bubbles with raw water. The uneven distribution of the phases seen in Figure 39 provide

an explanation for the great difference prior researchers have noted in Peclet number for

perfectly vertical columns and slightly tilted columns. The slight column misalignment

introduced into CFD calculations causes the bubble plume to migrate toward the wall and

contributes to the non-uniform distribution of phases.

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0

0.01

0.02

0.03

0.04

0.05

g

(a) Gas volume fraction (b) Plume shape

Figure 39: Phase Distribution

Liquid superficial velocity vectors in the near-sparger region (the bottom 75 cm of

the reactor) at 4 gas flow rates are shown in Figure 40. At low gas flow rate (QG = 0.4

L/min) large recirculation regions appear on alternate sides of the plume, causing the

plume to rise in a wavy path. When gas flow rate is increased to 1.0 L/min, the bubble

plume diameter increases, squeezing the recirculation regions and resulting in faster

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down-flow of liquid near the column wall. Increasing gas flow rate to 1.5 L/min further

increases the velocity of the down-flowing liquid near the column wall. At a gas flow

rate of 2.0 L/min, distinct recirculating regions similar to those seen at a gas flow rate of

0.5 L/min appear, though somewhat smaller and with greater rotational speed.

(a) QG = 0.4 L/min (b) QG = 1.0 L/min (c) QG = 1.5 L/min (d) QG = 2.0 L/min

Figure 40: Water Velocity Vectors near the Diffuser

The recirculating regions seen in Figure 40 explain the asymmetric plume rise

observed during laboratory experiments – these large structures, once established, deflect

the bubble plume. These recirculation regions differ from those typically found in bubble

column reactors with non-flowing liquid phase. In countercurrent flow, the large scale

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flow structures move downward with the liquid flow, tending to swirl around the reactor

as they proceed. As these fluid structures progress, the bubble plume is deflected,

resulting in a chaotic bubble plume motion. The shapes and locations of large fluid

structures are strongly dependent on reactor geometry and the interaction between

downflowing liquid and bubble plume is also expected to be influenced by reactor

geometry. The boundary between the bubble plume and down-flowing liquid and the

preferential flow path for liquid are clearly seen in Figure 40. This segregation between

the phases is an impediment to mass transfer and provides a “Short-circuit” by which

some of the liquid phase passes quickly out of the reactor. In disinfection, this short

circuiting provides a path for pathogenic organisms to elude treatment.

Axial variation in mixing in the column is shown in Figure 41. Neglecting large-

scale fluid motion, local mixing intensity is approximately proportional to the square root

of the rate of turbulent energy dissipation (Droste 1997). Figure 41(a) shows contours of

turbulent kinetic energy dissipation on a column midplane and Figure 41(b) is a plot of

mean dissipation as a function of axial location. Average turbulent dissipation, kP , at

axial location k, is calculated by:

1 ,,g

elemnts#

1 ,,,g

i kiki

i kikiki

kA

APP

(63)

where Ai,k is area of element i at axial location k. Mixing is non-uniform both axially and

radially. Mixing is highest near the sparger (z < 0.5 m) and uniform in the rest of the

column, except near the top where entrance effects dominate the flow. Mixing intensity is

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high inside the bubble plume; poorly mixed regions are observed outside the bubble

plume. These results provide an explanation for early breakthrough of tracer at high gas

flow rates (seen in Figure 36) – the flow field is partitioned into a well-mixed portion

rising in the bubble plume and a poorly mixed stream flowing downward.

Figure 41: Spatial Variations in Mixing

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The observed variations in mixing along the axial extent of the reactor have mass

transfer implications. Near the sparger, though mixing in the bubble plume is intense,

liquid is rising in the bubble plume and has relatively high dissolved gas concentration;

the concentration gradient is low and mass transfer rate is low, despite intense mixing.

Away from the sparger mixing is uniform and the bubble plume is distributed more

evenly in the column. Based on these observations, local mass transfer rate near the

sparger is expected to be different from that away from the sparger. Currently, most

bubble column designs are based on an assumption that mass transfer is relatively

uniform in the reactor.

V.4 Influences of Inlet and Discharge Configurations

Most often in industrial and pilot scale ozone bubble contactors, liquid does not

enter the reactor opposing gas flow. Rather, it flows into the pilot reactor or chamber of a

full scale reactor perpendicular to the gas rise direction, as illustrated in Figure 42, a

schematic diagram of a full-scale ozonation reactor in current use in the Netherlands

(Smeets et al., 2006). Inlet hydrodynamics can exert a strong influence on the behavior

of the bubble plume(s) and the degree of mixing in the reactor. For example, for the

configuration shown in Figure 42, the cross-flowing water entering the dissolution

chamber is expected to deflect the bubble plume top toward the baffle wall and to

generate a large circulation in the dissolution chamber.

The impact of inlet and discharge configuration on the flow field in a

countercurrent flow bubble column was investigated via CFD modeling of a pilot scale

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ozone bubble column reactor operated by the Philadelphia Water Department (Charlton

2003). The Philadelphia Water Department evaluated ozone disinfection as an alternative

to chlorine for improved inactivation of Cryptosporidium parvum and reduced formation

of disinfection by-products (DBPs). The pilot study indicated that bromide

concentrations observed in Schuylkill River water gave rise to unacceptable bromate

concentrations when treated with ozone and alternative means for DBP control were

adopted.

Figure 42: Typical Intake Configuration for Countercurrent Full Scale Ozonation

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V.4.1 Philadelphia Water Department Pilot Disinfection Unit

The PWD pilot disinfection operation was comprised of 9 right circular

cylindrical reactors, each 15.2 cm (6 inches) in diameter arranged in series. Each column

was plumbed to allow operation in either cocurrent or countercurrent mode. Air or

ozonated air could be introduced into any of the first 4 columns in the pilot plant. Air or

ozonated air was sparged into the bottom of bubbled columns via a distributor plate.

Flow entered and was discharged from the columns via 6.4 cm (2.5 in) pipes, as seen in

Figure 43. In Co-current flow mode, the water entered the column perpendicular to the

column centerline approximately 10 cm above the sparger and exited the column

approximately 10 cm below the water surface. In countercurrent flow, the water entered

the reactor at the top and exited at the bottom.

Results of CFD analysis of the PWD pilot reactor are presented in Figure 43 -

Figure 45. In Figure 43, color contour plots of the gas volume fraction are shown for a

plane that passes through the reactor centerline. The water and gas flow rates for this

simulation were 37 L/min and 3.5 L/min. The CFD model of the first bubble column in

the PWD pilot reactor employed a mesh of 208,044 tetrahedral elements, with mesh

clustering near the intake and discharge ports, uniform bubble diameter of 2 mm and

specified medium turbulence intensity at the reactor water intake. All other model

components were the same as those described for the laboratory reactor model.

The inlet and discharge configurations result in deflection of the bubble plume

toward the discharge (at the reactor bottom) and away from the intake (at the top of the

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reactor). At the intake and discharge the distribution of phases is much less uniform than

in the middle of the reactor. This poor distribution of phases results in lower mass

transfer than is the phases were more evenly distributed, despite relatively energetic gas

phase. Velocity vectors showing superficial liquid velocity near the reactor intake and

discharge are plotted in Figure 44. A large vortex is present in the reactor in the portion

of the reactor opposite the discharge port. This vortex results in significant back-mixing

of the liquid phase and high dispersion, even though the phases are poorly distributed.

The water intake configuration promotes a strong flow of liquid along the column wall

directly opposite the intake.

Results of a virtual tracer study of the PWD pilot reactor operated in

countercurrent mode are presented in Figure 45. As expected based on the velocity

vectors plotted in Figure 44, the tracer flows quickly down the reactor wall opposite the

intake and discharge side until the tracer front reaches the large vortex in the bottom of

the reactor. In the bottom of the reactor, the vigorous back-mixing results in a region of

uniform tracer concentration, despite poor distribution of phases.

The importance of inlet and discharge configuration in determining the residence

time distribution and hydrodynamics of bubble column contactors is not unique to tall,

cylindrical columns such as those used by the Philadelphia Water Department – Ta and

Hague (2004) found that inlet and discharge configurations were the dominant factor in

the flow field for a right rectangular cylindrical bubble contactor with the inlet transverse

to the flow direction and with a much lower aspect ratio than the Philadelphia Water

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Department contactor. Since full scale reactors typically employ inlets and discharges

perpendicular to the flow direction, care should be taken in accounting for inlet and

discharge hydrodynamics in scaling from pilot to full scale.

Figure 43: Philadelphia Water Department Pilot Column Phase Distribution

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(a) Reactor Discharge Region (a) Reactor Intake Region

Figure 44: PWD Pilot Reactor Intake and Discharge Region Velocity Vectors

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NormalizedTracer

Concentration

Figure 45: PWD Virtual Tracer Study

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VI MASS TRANSFER STUDIES

Flow visualization and computational fluid dynamic studies were performed of

mass transfer in the laboratory bubble column reactor. These studies allowed

quantification of spatial variations in mass transfer in a simple cylindrical bubble column

reactor. The studies also demonstrated that, without a priori knowledge of mass transfer

coefficient and without calibration, a computational fluid dynamic model can be used to

predict phase distribution and mass transfer in countercurrent bubble column flow. Thus

CFD should be considered more reliable than currently-used models for scale-up of

bubble column reactors from pilot scale to full scale.

In this chapter, results from the ozone mass transfer visualization technique

described above are presented and a qualitative description of countercurrent

hydrodynamics and mass transfer in a cylindrical column is provided. Processed images

of indigo dye are then used for estimation of mass transfer rate, dispersion and entrance

region length for the bubble column operating at three liquid flow rates and two gas flow

rates. Images of indigo dye are compared with images generated using CFD and CFD is

compared to other countercurrent flow models. Finally, the impact of choice of mass

transfer submodel in a CFD model is quantified.

VI.1 Matrix of Mass Transfer Studies

Mass transfer visualization experiments were conducted at three gas flow rates

and three liquid flow rates. In all but one experiment, ozone generator voltage was

chosen to provide a wide variation in indigo dye concentration in the reactor while

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179

ensuring the indigo was not decolored anywhere in the reactor. In the single experiment

conducted at the highest gas flow rate, the indigo dye was decolored above the bottom of

the reactor. Though the images taken of that case could not be used in the estimation of

mass transfer rate or mixing, they did allow visualization of entrainment of indigo dye

into the bubble plume.

The mass transfer visualization experiments conducted are summarized in Table

21. Experiments run at the same gas and liquid flow rates are designated case A and case

B. The range of gas to liquid flow ratios used in experiments are typical of those used in

prior pilot studies and in full scale facilities (Mariñas et al., 1993; Owens et al., 2000).

Table 21: Mass Transfer Visualization Experiments

Tap waterflow rate(lpm)

Indigostock flowrate (lpm)

Net liquidflow rate,QL (lpm)

Gas flowrate, QG,(slpm) QG / QL Case

Ozonegeneratorvoltage

Discharge watertemperature (°C)

6 1 7 0.4 0.057 A 60 22

6 1 7 0.4 0.057 B 65 16

9 1.5 10.5 0.4 0.038 A 60 20

9 1.5 10.5 0.4 0.038 B 65 12

12 1.5 13.5 0.4 0.030 A 65 9

12 1.5 13.5 0.4 0.030 B 70 4.5

6 1 7 0.7 0.100 65 17

9 1.5 10.5 0.7 0.067 65 20

12 1.5 13.5 0.7 0.052 70 20

9 1.5 10.5 0.9 0.087 70 22

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VI.2 Ozone Mass Transfer Visualization Results

The indigo dye ozone mass transfer visualization technique allowed qualitative

and quantitative observations of the mass transfer process. In this section, images from

the mass transfer visualization technique are presented and the hydrodynamics of mass

transfer are described. Next, estimates of Peclet number and Stanton number are made

using radially-averaged indigo dye color data and the variation in these parameters with

column gas to liquid flow ratio is documented.

VI.2.1 Observations

The indigo dye mass transfer visualization technique yielded vivid images that

allowed direct observation of mixing and mass transfer in the laboratory reactor. As

described above, the influent indigo dye concentration and gas phase ozone concentration

were chosen to provide the widest possible variation in indigo dye color between the

reactor top and bottom but to ensure indigo dye was present in the reactor discharge.

Images showing indigo dye decoloration at gas to liquid flow rates of 0.06 and

0.03 are presented in Figure 46. The only processing performed on the two images in

Figure 46 was elimination of background variations in lighting. The light triangular mark

approximately 1/3 of the axial distance between the reactor bottom and top is the

manufacturer’s mark (physically present on the laboratory reactor wall). The sparger and

glass bead packing appear white in the images because there was no difference in color

between the indigo dye image and the background image from which it was subtracted.

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181

(a) Qg/QL= 0.06 (b) Qg/QL= 0.03

Figure 46: Indigo Dye Decoloration Images

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Both of the images shown in Figure 46 were taken while ozone was being fed to

the reactor and after the reactor reached quasi-steady state (as described in Chapter III).

Image (a) was taken at gas and liquid flow rates of 0.4 slpm and 7.0 lpm (gas to liquid

flow rate of 0.06), ozone generator voltage of 65 V and indigo dye inlet concentration of

5.5 mg/L. Image (b) was taken at gas and liquid flow rates of 0.4 slpm and 13.5 lpm (gas

to liquid flow ratio of 0.03), ozone generator voltage of 65 V and indigo dye inlet

concentration of 4.3 mg/L.

There are significant differences in the pattern of indigo dye decoloration

observed in Figure 46 (a) and Figure 46 (b). At high gas to liquid flow rate (Figure 46

(a)), there is a relatively sharp decline in indigo dye concentration near the top of the

reactor. Asymmetric flow of the indigo dye downward can be observed at the top of the

reactor and slightly below the manufacturer’s mark. Large swirls of dye (length scale on

the order of the column diameter) are observed throughout the reactor, particularly in the

bottom half of the reactor. At high gas-to-liquid flow ratios, in the bottom half of the

reactor, dye projected downward along the column wall and large eddies of dye-rich

liquid were entrained into the bubble plume, decoloring rapidly after entrainment. At a

low gas to liquid flow ratio (Figure 46 (b)), the decoloration of indigo dye is more

uniform in the liquid flow direction than at the high gas to liquid flow ratio.

In both images, the concentration of indigo dye appears to increase at the very

bottom of the reactor. This increase is more pronounced in the high gas-to-liquid flow

ratio and was observed in most of the images obtained during mass transfer visualization

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183

experiments. It is hypothesized that this increase is a result of the entrainment of indigo

dye-rich liquid outside the bubble plume into the large recirculating regions near the

sparger shown in Figure 40.

The progress of dye-rich eddies downward is shown more clearly in Figure 47. In

that figure, images 1 and 2 were both taken at quasi-steady state, approximately 20

seconds apart. Images were converted to grayscale and contrast was enhanced to

accentuate the indigo dye color. For the images in Figure 47, gas and liquid flow rates

were 0.9 slpm and 10.5 lpm, respectively, the ozone generator was operated at a voltage

of 70 V, and indigo dye intake concentration was 5.5 mg/L. These operating conditions

resulted in near complete discolorization of the indigo dye upstream of the discharge.

Complete discolorization produced images that show flow details very well.

Large eddies with high indigo dye concentration and with length scale on the

order of column diameter appear to flow downward outside the bubble plume core,

spiraling around the reactor as they proceed. As they descend these eddies are entrained

into the bubble plume and decolored rapidly. The images in Figure 47 indicate two

important mixing length scales: mass transfer from bubbles to liquid depends upon

mixing on the length scale of the order of the bubble diameter. Transport of “fresh”

liquid to the bubble plume from the bulk liquid phase depends on mixing on the length

scale of the column diameter. Figure 47 also indicates that even within the dispersed

bubble flow regime, discharge indigo dye concentration is unsteady, because the

transport of the large indigo-rich eddies is a time dependent random process. This

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184

observation is constituent with measurements of effluent ozone concentration in full-scale

ozone fine bubble contactors (Schulz and Bellamy 2000) and should be considered when

evaluating sample ozone residual concentration data for making Ct estimates.

(a) Image 1 (b) Image 2

Figure 47: Eddy Transport during Ozonation

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185

VI.2.2 Parameter Estimates

Images from mass transfer visualization studies were used to estimate mass

transfer rate and dispersion. The steps in this process were:

Processing of indigo dye images (subtraction of background and conversion to

greyscale);

Calculating radially averaged indigo dye concentration data from processed indigo

dye images;

Application of non-linear regression to determine the parameters of candidate models

for the fate and transport of indigo dye that produce the best fit of data from indigo

dye images; and

Comparison of fitted models to determine the model that best fit the data.

VI.2.2.1 One-Dimensional Indigo Dye Decoloration Models

As described above and observed by prior researchers (Rice and Littlefield 1987;

LeSauze et al., 1993), in the top portion of the laboratory reactor, indigo dye was

decolored more or less monotonically as the dye flowed downward. Near the sparger,

however, the dye concentration was nearly uniform, exception where large eddies of dye-

rich water flowing near the walls were entrained into the bubble plume. This tendency is

illustrated in Figure 48, which shows an image of indigo dye concentration along with a

plot of radially-averaged indigo dye concentration.

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186

0.4 0.5 0.6 0.7 0.8 0.9 1.0

1.0

0.8

0.6

0.4

0.2

Well-mixedzone

z*

CI*

Figure 48: Illustration of Well-Mixed Zone and Radially-Averaged Concentration

The gas and liquid flow rates corresponding to Figure 48 were 0.4 slpm and 13.5

lpm, respectively. The terms z* and CI* are nondimensional depth and dimensionless

indigo dye concentration, given by

H

zz * (64)

and

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187

0,

*

I

II

C

CC (65)

where z is depth from the water free surface, H is reactor height (from the

discharge ports to the water free surface), CI is indigo dye mass concentration and CI,0 is

indigo dye concentration at the liquid inlet.

Based on this observation, two models for indigo dye decoloration were proposed:

a single-zone model in which the dispersion and mass transfer coefficient were

assumed uniform in the reactor and

a two-zone model in which the portion of the reactor near the sparger was modeled as

a continuously stirred tank reactor (CSTR) and the rest of the reactor was modeled

using the 1-dimensional advection-dispersion-reaction (ADR) model.

Detailed derivation of expressions for indigo dye concentration for the one- and

two-zone models are provided in Appendix B and summarized below.

For the single-zone model, normalized indigo dye concentration is given by

**

111* zPPS

zSNSNe

eS

IeeSS eeSNeeP

PSNC

(66)

where NS is Stanton number, given by

;L

LS

U

HakN (67)

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188

S is stripping factor, given by

;L

G

U

UmS (68)

Pe is Peclet number, defined in equation 39 (repeated below)

D

HUP L

e (39)

and the parameter is given by

0,

0

0,

0 3

3

3

3 I

gO

L

G

O

I

I

gO

O

I

C

C

Q

Qm

M

MS

C

C

M

M (69)

In equations 37, 59 - 61, kL is liquid side mass transfer coefficient, a is specific surface

area, m is Henry’s law constant (dimensionless ratio of mass concentration in gas phase

to mass concentration in liquid phase), UG and UL are superficial gas and liquid flow

rates, MI and3OM are molecular weights of potassium indigo trisulfonate and ozone,

03 gOC is gas ozone concentration at the sparger, and CI,0 is indigo trisulfonate

concentration at the water intake. Measured water temperature ranged from 4.9° C to 22°

C over the course of mass transfer visualization experiments and Henry’s law constant

was calculated via the expression (Perry and Chilton 1973)

C5C51687

2.6

C5C5840

25.3log

TT

TTm (70)

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189

In the limit of NS Pe, the single zone expression for normalized indigo dye

concentration becomes

e

PzPee

I PeezPPC

ee

ePS

SN

111*

lim

1*

*

(71)

Two versions of the two-zone model were fit to experimental data. In one version

the Stanton number was assumed the same in zones 1 and 2 and only mixing differed

between the two zones. The indigo dye concentration for this model is given by

****

**

*

*2,

*

11

1

1

cSecS

ee

zSNzPzzSN

cSeS

e

zPI

zPI

eezSNPSN

P

eCeC

(72)

where Pe refers to the Peclet number in zone 1 (the top of the reactor), zc* is the

nondimensionalized critical depth and *2,IC is the dimensionless indigo dye concentration

in zone 2 (the well mixed zone) given by

data

c

n

niiI

cdataI

I CnnC

C ,

0,

*2,

11(73)

where ndata is the number of (pixels) in the indigo dye image and nc is the row

corresponding to the critical depth.

For the two-zone model in which different Stanton numbers were allowed in

zones 1 and 2, the expression for indigo dye concentration is

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190

*

1***

1

**

*21

*2,

*

11

1

1

cSecS

ee

zSNzPzzSN

cSeS

e

zPI

zPI

eezSNPSN

P

eCeC

(74)

where NS1 and NS2 are the zone 1 and zone 2 Stanton numbers. In the limit eS PSN 1 ,

the expression for indigo dye concentration becomes

*2

**

2,*

111

**

**

cS

zzPezP

IzP

IzSN

ezPeCeC

ce

ee

(75)

VI.2.2.2 Methodology for Determining Model Parameters

Model equations 58, 62, 65 and 66 were fit to radially-averaged indigo dye

concentration data from digital photographs of mass transfer visualization experiments.

Fits were made using the nls (nonlinear least squares) utility in the R programming

language (The R Foundation 2006). After models were fit to data, independence was

assessed via runs tests (Manly 1997). Data were considered independent unless

independence could be rejected with 95% confidence.

When dependency was encountered, a subset of data was taken from the original

data set, best fit parameters were again determined and independence was again assessed.

Two sampling methodologies were assessed when selecting subsets from the original

data set. In one, a random sample of ndata/j points was taken from the original data set,

where ndata was the number of data points (rows) in the original data set and j took the

values 2, 4, 8, 16, 20, 24, 28, 32, 36, 40, 44, 48, 52, 56, 60 and 64. In the second

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191

sampling methodology a systematic sample was taken in which the subset consisted of

each jth data point where j took the values 2, 4, 8, 16, 20, 24, 28, 32, 36, 40, 44, 48, 52,

56, 60 and 64. In all cases the systematic sampling resulted in elimination of dependence

at lower values of j than the random sampling. Reducing the number of data points did

not result in significant changes in parameter estimates. In all cases, independence could

be demonstrated for the two-zone model (usually after the number of data points in the

sample was 20 times less than that in the original data set). Independence could not be

demonstrated for any cases for the single-zone model. Thus, the two zone model was

considered the more appropriate model and parameter estimates were taken from the two-

zone model.

In two zone models, the critical depth, zc*, was determined as follows. The best

fit parameters and sum of the squares of the errors were determined for all zc* (0.5,

1.0). The critical depth was taken to be the value that gave the lowest sum of squares of

errors. The minimum sum of the squares of the errors was usually readily identifiable. A

typical plot of sum of the squares as a function of index of critical depth is provided in

Figure 49. In digital images, each row of pixels corresponds to a value of z*, so in Figure

49, the index nc is the row number corresponding to the critical depth zc. For the plot

shown, there was a total of 60 data points and the critical depth was determined to be at

the 44th data point.

An R-language script used for determination of two-zone model best fit

parameters and for performing a runs test of the fitted model is provided in Appendix D:

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192

Similar scripts were written for the one zone model and for versions of the models in

which the Peclet and Stanton numbers were equal.

30 35 40 45 50 55 60

0.0

02

20

.002

40

.002

60.0

028

nc

SS

E

Figure 49: Identification of Best Fit Critical Depth

VI.2.2.3 Parameter Estimates

Processed images, best-fit models and parameters corresponding to best fit

models for each mass transfer visualization experiment are presented below. For each of

the indigo dye experiments, two images and plots showing 1- and 2-zone best fit models

are shown in Figure 51 - Figure 59. Both color (blue) and grayscale images are provided,

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since the color images provide greater detail in the variation of indigo dye color. Along

with reactor images, plots of best fit 1-zone and 2-zone models are provided. In all cases,

independence could not be demonstrated for the one-zone model; the one-zone plots are

included in Figure 51 - Figure 59 for contrast with best fits of the two-zone model and to

document the trends in data that gave rise to data dependence. Data dependence is

manifested in either periodic variation of the data around the model (such as seen in

Figure 53 (c)) or significant deviation of the model from the data at the top and bottom of

the reactor (such as seen in Figure 52 (c)).

Several general observations can be made based on Figure 51 - Figure 59. First,

in all cases, in the top of the reactor the indigo dye concentration decreases steadily as the

water progresses downward. Second, the rate of decrease of indigo dye in the bottom of

the reactor is always less than that in the top of the reactor (though not necessarily zero,

as would be observed in a true CSTR). Third, in several cases (Figure 53, Figure 56,

Figure 58 and Figure 59) there is an upturn in indigo dye concentration at the very bottom

of the reactor. One explanation for this upturn is that dye-rich water flowing along the

column walls is backmixed into the column as the water is entrained into the large eddies

near the sparger (as seen in Figure 40). As seen later in this chapter, CFD also predicts

there is a region of high indigo concentration at and below the sparger depth. Finally, the

inability to demonstrate independence for the single zone model is related to large length

scale oscillations in indigo dye concentration around the trend line. These oscillations are

not surprising, given the observation of large dye-rich eddies flowing downward in the

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reactor, and indicate that time series analysis of radially-averaged indigo dye

concentration data might yield quantitative data on large scale mixing processes.

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Figure 50: Mass Transfer Visualization, Qgas = 0.4 slpm, QL = 7.0 lpm, Case A

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Figure 52: Mass Transfer Visualization, Qgas = 0.4 slpm, QL = 7.0 lpm, Case B

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Figure 53: Mass Transfer Visualization, Qgas = 0.4 slpm, QL = 10.5 lpm, Case A

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Figure 54: Mass Transfer Visualization, Qgas = 0.4 slpm, QL = 10.5 lpm, Case B

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Figure 55: Mass Transfer Visualization, Qgas = 0.4 slpm, QL = 13.5 lpm, Case A

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Figure 56: Mass Transfer Visualization, Qgas = 0.4 slpm, QL = 13.5 lpm, Case B

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Figure 57: Mass Transfer Visualization, Qgas = 0.7 slpm, QL = 7.0 lpm

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Figure 58: Mass Transfer Visualization, Qgas = 0.7 slpm, QL = 10.5 lpm

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Figure 59: Mass Transfer Visualization, Qgas = 0.7 slpm, QL = 13.5 lpm

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Best fit parameters for each mass transfer visualization experiment are presented

in Table 22. In Table 22, the sample size at which independence could not be rejected

with 95% confidence was ndata / j where ndata is the number of data points in the full data

set. In general, Peclet number estimates were found to vary more widely than estimates

for Stanton number and length of the entrance region. In one case (gas flow rate of 0.4

slpm, liquid flow rate rate of 10.5 lpm, case B) the zone 2 Stanton number was estimated

to be zero. This indicates that the change in indigo color observed in the top of the

reactor can be attributed solely to mixing and that all significant mass transfer takes place

in the well-mixed zone in the bottom of the reactor.

Table 22: Best Fit Parameters

Qg (slpm) QL (lpm) Case j Pe NS1 NS2 zc*

0.4 7.0 A 24 1.49 0.29 0.29 0.266

0.4 7.0 B 56 1.93 0.43 0.43 0.282

0.4 10.5 A 32 5.77 0.16 0.025 0.226

0.4 10.5 B 16 1.66 0.19 0.00 0.240

0.4 13.5 A 16 2.04 0.14 0.14 0.173

0.4 13.5 B 36 7.76 0.10 0.10 0.216

0.7 7.0 24 1.91 0.96 0.96 0.396

0.7 10.5 28 1.52 0.35 0.35 0.266

0.7 13.5 24 1.93 0.38 0.38 0.219

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Peclet number, Stanton number and critical depth were found to correlate with the

ratio of gas to liquid flow rates. Figure 60 shows the variation in entrance region length

(1 - *cz ) with gas to liquid flow ratio. Estimates based on data from experiments

conducted at a gas flow rate of 0.4 slpm are shown as solid diamonds and those based on

experiments at a gas flow rate of 0.7 slpm are shown as unfilled squares. Entrance region

length increases steadily with increasing gas to liquid flow ratio for the gas and liquid

flow rates used in this study. This result indicates that high gas to liquid flow rates result

in greater mixing of the liquid phase (primarily through the formation of large vortices in

the vicinity of the sparger and attendant backmixing of the liquid phase) but less uniform

distribution of the phases. In a more complex reactor geometry than that of the

laboratory rector used in this study, uneven distribution of phases creates the potential for

short-circuiting of the liquid phase in the bubble column and could result in significant

variations in ozone residuals, as has been observed in full-scale ozonation reactors

(Schulz and Bellamy 2000).

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0

0.05

0.1

0.15

0.2

0.25

0.3

0.35

0.4

0.45

0.02 0.03 0.04 0.05 0.06 0.07 0.08 0.09 0.1 0.11

Gas to Liquid Volumetric Flow Ratio

En

tra

nce

reg

ion

len

gth

(%o

fre

act

or

hei

gh

t)

0.4 slpm

0.7 slpm

Figure 60: Variation of Entrance Region Length with Gas to Liquid Flow Ratio

As expected, zone 1 Stanton number increases with gas to liquid flow ratio, as

seen in Figure 61. Higher gas flow rates produce more bubbles, resulting in greater

dispersion (in the bubble wakes) and higher specific surface area (a). Had gas phase

holdup been measured during mass transfer visualization studies, the relative importance

of these two changes (increased dispersion and increased specific surface area) could

have been ascertained.

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0

0.2

0.4

0.6

0.8

1

1.2

0 0.02 0.04 0.06 0.08 0.1 0.12

Gas to Liquid Volumetric Flow Ratio

Sta

nto

nN

um

ber

Figure 61: Variation of Zone 1 Stanton Number with Gas to Liquid Flow Ratio

The variation of zone 1 Peclet number with gas to liquid flow ratio is shown in

Figure 62. As noted in Table 22, there was wide variation in Peclet number estimates

from indigo dye image analysis, indicating high uncertainty in Peclet number estimates,

especially at low gas-liquid flow ratios. In general, data follow the trends in Peclet

number determined via RTD studies and CFD analyses shown in Figure 37, except for

one estimate of Peclet number at the lowest gas to liquid flow rate. Images and best fit

model for the case with the unexpectedly low Peclet number are found in Figure 56.

Images and best fit model for the other case at the lowest gas to liquid flow ratio are

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found in Figure 55. The only difference in operating conditions between the two cases is

the ozone generator voltage: the voltage for the low Peclet number case was 70 V and

that for the other case was 65 V. Based on the images in Figure 56, it is possible that

some of the liquid phase was completely decolored for the case run at the higher ozone

generator voltage and this may have made the Peclet number estimate less accurate.

0

1

2

3

4

5

6

7

8

0 0.02 0.04 0.06 0.08 0.1 0.12

Ratio of Gas to Liquid Volumetric Flow Rate

Pec

let

Nu

mb

er

Figure 62: Variation of Zone 1 Peclet Number with Gas to Liquid Flow Ratio

The most significant findings and observations from the experimental mass

transfer studies are that:

The mass transfer and mixing near the sparger (in the “entrance region”) differ from

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those in the rest of the reactor.

The entrance region length can be determined using the indigo dye mass transfer

visualization technique.

The entrance length increases with increasing gas to liquid flow ratio.

Although the entrance region liquid phase is well-mixed, distribution of phases in the

entrance region is poor.

Stanton number increases with increasing gas to liquid flow ratio, likely because of

specific surface area and turbulent dispersion increases.

Peclet number trend is similar to that measured in RTD studies and predicted in CFD

studies.

VI.3 CFD Mass Transfer Modeling Results

As described above, CFD was used to predict ozone mass transfer and fate and

transport of indigo dye. Recapping important CFD model features, bubbles were

assumed monodisperse with a diameter of 2.5 mm, bubble drag was estimated using the

Grace drag model (Clift et al., 1978), mass transfer rate was estimated using the Kawase

mass transfer relation (Kawase and Moo-Young 1992) and the indigo-ozone reaction was

assumed sufficiently fast that there was no accumulation of dissolved ozone. The CFD

model was run to allow comparison of predictions with results of four mass transfer

visualization experiments:

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QG = 0.4 slpm, QL = 7.0 lpm, case A

QG = 0.4 slpm, QL = 13.5 lpm, case A

QG = 0.7 slpm, QL = 7.0 lpm, and

QG = 0.7 slpm, QL = 13.5 lpm.

Direct comparison was made between indigo dye concentrations predicted by

CFD and measured concentrations from samples drawn from the reactor. Samples were

drawn from the reactor centerline from regularly spaced sample ports on the laboratory

bubble column. The sample ports were sealed with Teflon seals held in place by fittings

that allowed samples to be drawn from the sample centerline by 25 cc glass syringes

outfitted with 3 inch (7.62 cm) hypodermic needles. Sample locations are shown in

Figure 63.

Prior to sampling, the reactor was run at steady water and gas flow rates and

ozone dose for more than three hydraulic residence times. Samples were drawn from one

sample port at a time, beginning with the top port and proceeding to the bottom.

Individual samples required up to 20 seconds to draw and the entire sampling process

took approximately 2 minutes. Sample sizes were small (between 11 and 15 cc).

Samples were diluted with enough milli-Q water to make the total sample volume 40 cc

(the minimum sample volume for the 1 inch diameter (2.5 cm) spectrophotometer cells

used) and absorbance was measured using a spectrophotometer. Absorbance of samples

was measured at 500 nm and indigo concentration was calculated for samples using the

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calibration curve described in Chapter III and accounting for dilution.

Figure 63: Sample Locations

Sample and CFD normalized indigo dye concentrations are compared in Figure

64. CFD results agree very well with sample concentrations at the bottom and top of the

reactor, but are consistently lower in the center of the reactor. It is difficult to assess the

CFD model based on this comparison. As described above, flow in the reactor is

decidedly three dimensional and transient

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0

0.1

0.2

0.3

0.4

0.5

0.6

0.7

0.8

0.9

0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9

z*

CI*

CFD

Experimental

Figure 64: Predicted and Measured Indigo Dye Concentrations

Color contours and grayscale contours from CFD analyses are presented next to

processed experimental indigo dye images in Figure 66 - Figure 69. Qualitatively, the

consumption of indigo dye in the CFD images is very close to that of the experimental

image. Differences in indigo dye concentration radial distribution between the

experimental and CFD are related to differences between how the CFD image and the

image captured on camera were generated. The experimental image is a two dimensional

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image of the average indigo concentration at a particular location (r, z) on the image

background, as illustrated in Figure 65. The CFD image shows indigo contours at a plane

passing through the centerline of the reactor. Additionally, portions of bubble surfaces

appear as dark spots in the experimental image, making the bubble plume look slightly

darker than it should. As described in the experimental methods indigo dye concentration

calibration portion of this thesis (section III.3.4), the indigo dye calibration curve

(relating indigo dye concentration to image pixel color) was developed for images with

bubbles. In CFD images, no bubbles are present and this difference results in minor

differences between CFD and experimental images of indigo concentration.

Image

Image

(a) Image Location, Experimental Image (b) Image Location, CFD

Figure 65: Image Location, Experimental Images and CFD

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The impact liquid flow rate has on spatial distribution of mass transfer can be seen

through comparison of Figure 66 and Figure 67. The gas flow rate was the same for both

cases (0.4 slpm) and the liquid flow rates are 7.0 lpm and 13.5 lpm, respectively. In the

high gas to liquid flow ratio case (Figure 66), indigo dye is decolored nearly to the top of

the reactor, with the lowest indigo concentration water found in the bubble plume slightly

above the sparger. At high liquid flow rate, the region in which indigo dye is decolored

is much shorter, reaching only the reactor mid-height. In the high liquid flow case, there

is vigorous backmixing of the liquid phase near the sparger and ozone is stripped from

the gas phase rapidly near the sparger as a result of this mixing. At a gas flow rate of 0.7

slpm, the trend of mass transfer occurring over a greater portion of the reactor at the low

liquid flow rate (Figure 68) than at high liquid flow rate (Figure 69) is again observed.

Comparing the CFD and experimental images, some of the flow structure

observed in the experimental images is not seen in the CFD images. For example, Figure

69, large swirls of high indigo dye concentration water are observed in the bottom half of

the reactor. The absence of these eddies in the CFD results is a result of the choice of

turbulence model. Had a LES (large eddy simulation) model been chosen instead of the

- implemented, these eddies might have been identified, though a finer mesh and

smaller time step would have been required.

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(a) Experiment (b) CFD, Color Contours (c) CFD, Grayscale

*IC *

IC

Figure 66: Experimental and CFD Indigo Dye Image, QL = 7.0 lpm, QG = 0.4 slpm

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(a) Experiment (b) CFD, Color Contours (c) CFD, Grayscale

*IC *

IC

Figure 67: Experimental and CFD Indigo Dye Image, QL = 13.5 lpm, QG = 0.4 slpm

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(a) Experiment (b) CFD, Color Contours (c) CFD, Grayscale

*IC *

IC

Figure 68: Experimental and CFD Indigo Dye Image, QL = 7.0 lpm, QG = 0.7 slpm

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Figure 69: Experimental and CFD Indigo Dye Image, QL = 13.5 lpm, QG = 0.7 slpm

(a) Experiment (b) CFD, Color Contours (c) CFD, Grayscale

*IC *

IC

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To allow direct comparison of CFD predictions with data from mass transfer

visualization images, CFD predictions for indigo dye concentration were averaged on

horizontal planes (area-weighted averaging) and plotted along with radially-average

indigo dye data. The results of this comparison are plotted in Figure 70- Figure 73.

Figure 70 shows a plot of CFD and experimental average indigo dye concentrations

measured/calculated at a gas flow rate of 0.4 slpm and a liquid flow rate of 7.0 lpm. The

CFD model predicts the slope of the experimental indigo dye curve quite well, though the

CFD results are off-set from the experimental results. Figure 71 compares measured and

predicted indigo dye concentration at a gas flow rate of 0.4 slpm and a liquid flow rate of

13.5 lpm. Again, the CFD results have the same slope as the experimental results, but are

significantly off-set from the experimental values. Figure 72 compares measured and

predicted indigo dye concentration at a gas flow rate of 0.7 slpm and a liquid flow rate of

7.0 lpm. The CFD predictions are in worse agreement with experimental values at these

operating conditions than for any other cases, though the CFD model predicts the net

indigo dye consumption in the reactor fairly accurately. It appears the CFD model does

not adequately model the mixing zone near the sparger. Finally, Figure 73 compares

measured and predicted indigo dye concentration at a gas flow rate of 0.7 slpm and a

liquid flow rate of 13.5 lpm. Again, the CFD model predictions appear offset from the

experimental values.

One plausible explanation for the offset observed between observed and predicted

indigo dye concentrations is uncertainty in reactor influent indigo dye concentration.

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Indigo dye solution was delivered to the influent plumbing via a peristaltic metering

pump. Prior to experiments, the pump was calibrated via measurement of water flow rate

and comparison with pump read-out. These measurements were made with the pump

discharging to atmospheric pressure through a short length of tubing. It is possible that,

with the pump delivering water to the column, the pump delivery rate differed from that

measured during calibration studies or that the pump delivery rate varied during

experiments due to chaffing of the tube through indigo dye solution was delivered.

Figure 70: Comparison of CFD and Experimental Indigo Dye Concentration Data,Q6=0.4 slpm, QL=7.0 lpm

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Figure 71: Comparison of CFD and Experimental Indigo Dye Concentration Data,Q6=0.4 slpm, QL=13.5 lpm

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Figure 72: Comparison of CFD and Experimental Indigo Dye Concentration Data,Q6=0.7 slpm, QL=7.0 lpm

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Figure 73: Comparison of CFD and Experimental Indigo Dye Concentration Data,Q6=0.7 slpm, QL13.5 lpm

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VII CRYPTOSPORIDIUM INACTIVATION AND BROMATE FORMATION INA FULL-SCALE REACTOR

A rough CFD model was developed to demonstrate CFD prediction of mass

transfer, Cryptopsoridium parvum inactivation, bromate formation and ozone decay in a

full scale reactor. Here, rough means 2-dimensional and with a relatively coarse mesh.

Because the intent of the full scale modeling effort was demonstration and not rigorous

prediction, the rough model was deemed adequate. Had more accurate results been

required, a more detailed CFD study would have been conducted more methodically and

would have included a mesh sensitivity analysis and validation with experimental data.

VII.1 Description of Full Scale Reactor

The full-scale reactor modeled in this demonstration is the Alameda County

Water District (ACWD) ozone contactor located in Fremont, CA. Design and operating

condition details for the reactor were drawn from the study by Tang et al. (2005). In that

study, the authors assessed the ability of the one-dimensional advection-dispersion-

reaction model (ADR) to predict Cryptosporidium parvum inactivation and bromate

formation in a full scale reactor. The authors determined that the ADR model, when

calibrated with dispersion data from tracer studies, provided “good” agreement with

experimental data (calculated v. predicted ozone residual, Cryptosporidium parvum

surrogate concentration and bromate concentration) for most cases, though for at least

two operating conditions predicted ozone residual was significantly different from

measured residual. The authors suggested poor agreement in those cases might have

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been the result of variation in water quality during experiments or might have been

related to their model’s simplifying assumptions. They also suggested that backmixing

strongly influences bromate formation, which suggests the ADR model, which does not

formally incorporate backmixing, may not be the optimal model for use in predicting

bromate formation in full scale reactors.

A schematic diagram showing the full-scale contactor is provided in Figure 74.

Reactor dimensions and other design data were taken from a published study of the

hydrodynamics and disinfection efficiency of the full scale reactor (Mariñas et al., 1999).

The two, two-phase chambers are operated in countercurrent mode. Based on data

presented in one study of the full scale reactor (Tang et al., 2005), the ozone generator

feed gas is dried air and gas to liquid flow ratio in the reactor varied between 0.083 and

1.4. Gas was injected through fine pore diffusers. The shape and spacing of the diffusers

were not reported.

In the rough (two dimensional) CFD model developed for the reactor shown in

Figure 74, several simplifications of reactor geometry were made. The simplifications

were made because detailed design data were not available. Had these data been

available, developing a more accurate model geometry and improved mesh would have

been straightforward and would not have resulted in significant increases in the CPU time

required to generate solutions.

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6.77 m

2.36m

0.92m

2.44m

0.92m

0.92m

0.92m

1.98m

1.98m

1.98m

0.84m

Waterintake

Diffusers

Discharge

Figure 74: ACWD Full Scale Reactor Schematic Diagram

VII.2 Full Scale Reactor CFD Model

VII.2.1CFD Model General Features

The major features of the full scale reactor CFD model were largely the same as

those of the laboratory reactor CFD model:

Two phase flow was modeled using an Eulerian-Eulerian treatment.

Bubbles were assumed monodisperse with a bubble diameter of 2.5 mm.

Bubble drag was calculated using the Grace drag model and ozone mass transfer was

calculated using the Higbie mass transfer model.

Dirichlet (specified normal velocity) boundary conditions were used for the water and

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gas intakes; a pressure boundary condition was applied at the water discharge. The

water free surface was specified as a “degassing” boundary (free-slip boundary for

the liquid flow, zero gradient boundary for the gas phase).

A schematic diagram showing the CFD model is presented in Figure 75.

Symmetry planeWater inlet(specified normalvelocity andCryptosporidiumparvum numberdensity)

Gas inlet (specifiednormal velocity andO3 concentration)

Degassing boundary at water surface

Water discharge(specifiedpressure)

Figure 75: Full Scale Reactor CFD Model Schematic Diagram

To reduce computation time, only half the reactor was modelled and a symmetry

boundary condition was imposed at the reactor midplane, as shown in Figure 75. A

relatively coarse unstructured mesh with a total of 704,200 elements was employed.

Elements were clustered near the inlet, the spargers and the underflows/overflows of the

baffles.

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VII.2.2Cryptosporidium Inactivation and Bromate Formation Submodels

In the CFD model, scalar transport and reaction rate expressions were included

for ozone decay, ozone demand (by natural organic matter [NOM]), bromate formation

and Cryptosporidium parvum inactivation. Reaction rate expressions for all of these

constituents were those reported by Tang (2005) and presented below.

Ozone demand was modeled with first-order kinetics and, based on batch ozone

decay studies, the decay constant was -1s001.0011.03

Ok . The authors modeled

bromate formation as first order with respect to ozone concentration. Based on semi-

batch ozonation studies, the rate constant for bromate formation was estimated to be 9.4

10-5 s-1. Though the bromate formation model and rate constant are consistent with data

collected in batch experiments, their utility for waters other than those tested seems

unlikely, since the bromate formation rate is not dependent on raw water bromide or

ammonia concentrations.

C parvum inactivation was assumed to follow Chick kinetics (overall second

order, first order in both ozone concentration and C parvum oocyst density). Based on Ct

values in the LT2ESWTR (Table 1), the rate constant was TNk 097.10917.0 , where T

is temperature in °C.

Rate expressions for ozone decay, ozone demand, bromate formation and C.

parvum inactivation are summarized in Table 23.

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Table 23: Rate Expressions and Constants, Full Scale CFD Model

Reaction Rate expression Rate constant Notes

Ozonedecay 33

3

OO

OCk

dt

dC

-1s001.0011.03

Ok Batchexperimentsperformed at20°C

Ozonedemand NOMNOM 3

3 CCkdt

dCO

O

s-mg/L16.020.3NOM k Approximationdeveloped toensure demandoccurs muchfaster thandecay andinactivation

Bromateformation 33

3

BrO

BrO

OCkdt

dC

-15BrO s109.4

3

k Developedbased on batchexperiments.Initial bromideconcentrationnot reported

C. parvuminactivation NCk

dt

NdON 3

min-mg/L097.10917.0

3O

TNk Based on Ct

tables ratherthan batchexperiments

VII.3 Phase Distribution and Flow Field

Gas volume fraction contours predicted by the CFD model for the reactor

operating at a gas flow rate of 404 standard cubic meters per hour and a liquid flow rate

of 15.5 MGD (2.01 m3/s) are presented in Figure 76 -Figure 78. Gas volume fraction is

the volume occupied by gas within a given reactor volume. Figure 76 shows gas volume

fraction on a vertical plane at the midsection of the computational domain. The bubble

plumes from the individual diffusers do not rise straight upward. Rather, they are drawn

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toward the reactor headwall and coalesce as they rise. The tendency of bubble plumes to

be drawn toward walls and coalesce is consistent with the experimental observations of

Freire et al. (2002). Another factor in the deflection of the bubble plume toward the

headwall is the large clockwise circulation generated in the dissolution chamber by the

horizontal introduction of water to the chamber. This phenomenon is illustrated below.

Figure 76: Gas Volume Fraction Contours, Full Scale Reactor, Vertical Plane

The distribution of gas on a horizontal plane near the sparger and on a horizontal

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plane at the midheight of the reactor are shown in Figure 77 and Figure 78, respectively.

These figures show the migration of the bubble plume toward the center of the reactor

(due to coalescence of bubble plumes) and the presence of large vortices (diameter on the

order of the chamber length) in the dissolution chamber. The gas volume fraction

contours show a non-uniform and three dimensional distribution of gas in the reactor.

Figure 77: Gas Volume Fraction Contours, Full Scale Reactor, Horizontal Planenear the Spargers

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Figure 78: Gas Volume Fraction Contours, Full Scale Reactor, Horizontal Plane atthe Reactor Mid-height

Superficial velocity vectors on a vertical plane in the first 6 and last 6 chambers of

the reactors are shown in Figure 79 and Figure 80, respectively. In the vector plots, the

magnitude of the vector is indicated by its color and vectors were not projected onto the

plane.

In the ozone dissolution chamber (with the diffusers on the bottom, the

momentum of the influent water stream creates several large recirculations whose length

scales are on the order of the chamber width, as seen in Figure 79. There is a strong

upward flow along the reactor headwall and a strong downward flow of liquid at the

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upstream face of the first baffle. In the second large chamber, circulation is also

pronounced and water follows a serpentine path as it traverses the reactor. In subsequent

chambers (shown in Figure 80) the water flow path becomes better defined, tending to

flow preferentially at the upstream face of each baffle. The hydrodynamics illustrated in

Figure 80 deviate significantly from plug flow. In the final 5 chambers the main water

flow path occupies less than half the available cross sectional area and there are large

recirculating regions present in each chamber. As shown below, the presence of the

preferential flow path results in short circuiting of pathogens past treatment and the

presence of recirculating regions results in prolonged contact between bromide and ozone

and contributes to bromate formation.

Tracer studies performed by Tang et al. indicate that in the AWCD ozone bubble

contactor, the ozone dissolution chambers behave as CSTRs. This result supports the

approach proposed by Lev and Regli (1992b) of treating bubbled chambers as CSTRs in

assigning Ct credit. This result also indicates that conditions conducive to higher than

expected bromate formation exist (Tang et al., 2005), though in the prior study no

rigorous modeling or experimental work provided conclusive evidence that these

recirculating regions are indeed bromate formation “hot spots.”. The fluid recirculating

in the center of the dissolution chambers has a high residence time and potentially a high

ozone concentration.

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Figure 79: Water Superficial Velocity Vectors, Chambers 1 - 5, Full Scale Reactor

Like serpentine horizontal reactors, the 180 turns employed in the full scale

reactor design produce dead zones and large recirculations that reduce the effective

chamber cross sectional area and cause flow to deviate from plug flow, even in the

narrow chambers in which net water flow is upward. To improve non-ideal

hydrodynamics such as those seen in Figure 79 and Figure 80, engineers usually modify

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under-over baffle reactors by modifying baffle spacing (Cockx et al., 1999; Do-Quang et

al., 1999), modifying baffle gap distance (between the baffle and reactor floor) (Henry

and Freeman 1995), or by adding partial baffles that may be solid or perforated

(Heathcote and Drage 1995).

Figure 80: Water Superficial Velocity Vectors, Chambers 6 - 10, Full Scale Reactor

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Figure 81: Water Superficial Velocity Vectors, Full Scale Reactor, HorizontalPlane, Chambers 1 – 4, Projection Tangential to Plane

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Figure 82: Water Superficial Velocity Vectors, Full Scale Reactor, HorizontalPlane, Chambers 5 – 10, Projection Tangential to Plane

VII.4 Inactivation and Comparison to Log Credits from Ct Models

CFD predictions for ozone residual, bromate concentration and Cryptosporidium

oocyst number are presented in Figure 83, Figure 84 and Figure 85, respectively.

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Figure 83: Dissolved Ozone Concentration Contours, Full Scale Reactor

As measured in the full scale contactor (Tang et al., 2005), ozone residual at the

reactor discharge is less then 0.05 mg/L. The predicted ozone residual profile seen in

Figure 83 indicates that full advantage is not being used of the reactor volume. Because

no Ct credit is awarded for the first chamber (the only chamber with a high discharge

ozone residual), the only chamber contributing significantly to Ct is the second chamber

in which ozonated air is bubbled. From a Ct credit standpoint, a better operating

condition would be application of only enough ozone to overcome fast demand in the

first chamber and increasing ozone application in the second bubbled chamber. This

approach would result in higher ozone residual in the last 6 chambers of the reactor. For

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the first ozone dissolution chamber, the regulatory approach of not allowing any

disinfection credit presents a disincentive to good design (i.e., ozone application in the

two chambers that maximizes transferred dose and mixing) and is inconsistent with the

observation that significant disinfection can take place in a chamber that has low or no

measurable ozone residual in its effluent (Xu et al., 2002). Regardless of the point of

application of ozone, ozone decay is a serious problem in this reactor.

Because bromate formation rate was modeled as first order with respect to ozone

residual, bromate contours, shown in Figure 84, are similar to ozone contours. The small

region of low bromate concentration water in the discharge pipe is a result of the choice

of an entrainment boundary condition. For an entrainment boundary, pressure gradient is

set equal to zero and concentration of scalar species for fluid flowing into the boundary is

specified (in this case, influent bromate concentration was set equal to zero). Because the

low bromate concentration is confined to the discharge pipe, the boundary condition does

not influence conditions within the reactor and is considered adequate.

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Figure 84: Bromate Concentration Contours, Full Scale Reactor

Recirculating regions are bromate-formation hot spots. This is evident in the

bubbled chambers, both of which have large high bromate concentration regions in their

centers. Bromate formation in the last 5 chambers of the reactor is minimal, because

ozone residual is low. Predicted bromate formation does not exceed the MCL of 10

g/L, though if higher ozone residual were realized in the reactor, the production of

bromate would be higher.

Cryptosporidium parvum density contours, seen in Figure 85, indicate that

log removal of microorganisms is high for water detained in recirculations in the two

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bubbled chambers and

significant short circuiting exists non-bubbled chambers.

The first observation is consistent with the assumptions used in development of

methodology for determining reactor Ct. The second observation indicates that, despite

their common use, under-over baffled reactors employing 180 turns are prone to dead

zones in the corners of the turns and large recirculations in all chambers. These dead

zones and recirculations reduce the volume of reactor available for the main liquid flow

and promote short circuiting. Short-circuiting, in turn, reduces contact time between

microorganisms and disinfectant.

Suboptimal hydrodynamics related to flow through 180 turns occurs in single-

phase serpentine chlorine contactors and other chemical disinfection processes as well as

in ozone bubble contactors. Systematic study of design modifications that improve

hydraulics in such arrangements would be a general benefit to the water treatment

industry.

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Figure 85: Cryptosporidium parvum Density Contours, Full Scale Reactor

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VIII CONCLUSIONS AND DISCUSSIONS

VIII.1 Summary of Major Findings

Three gas flow rate ranges within the ideal bubbly flow regime were identified in

which the variation in Peclet number with gas flow rate differed. At low gas flow

rates, Peclet number falls sharply with gas flow rate. At intermediate gas flow rates

Peclet number does not vary with gas flow rate. At high gas flow rate Peclet number

falls with increasing gas flow rate.

CFD “virtual tracer” studies agreed very well with measured tracer concentrations.

CFD analyses predict large vortices are present at the column walls in the vicinity of

the sparger. These vortices cause back-mixing of the liquid stream and elongate as

gas-to-liquid flow ratio is increased.

CFD and mass transfer visualization experiments demonstrated that mixing is non-

uniform in the column. High-intensity mixing occurs at the bottom of the reactor,

which may be regarded as a completely mixed reactor. The length of this well-mixed

region increases with increasing gas-to-liquid flow ratio.

Outside the well-mixed zone, Stanton number increases with increasing gas-to-liquid

flow ratio.

VIII.2 Details of Major Findings

Two series of experiments were conducted to quantify mixing in countercurrent

bubbly flow, investigate spatial variations in mixing and mass transfer and explore the

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advantages of CFD over lower fidelity models such as the ADR and CSTR reactor

models for adequately reproducing phenomena observed in experiments. The anticipated

benefits associated with these goals were improved bubble contactor designs more

consistent with countercurrent hydrodynamics and better modeling leading to informed

management of acute and chronic health risks associated with drinking water

contaminants.

Tracer studies performed over a range of gas flow rates identified three gas flow

rate ranges in which mixing (Peclet number) variation with gas flow rate differed. For

gas flow rate below 1.0 slpm, Peclet number fell sharply with increasing gas flow rate. In

the gas flow range 1.0 to 2.25 slpm, Peclet number remained constant at 3.0. This

finding was consistent with that of one prior study of mixing in countercurrent flow

bubbly flow. Above gas flows of 2.25 slpm, Peclet number fell with increasing gas flow

rate, following trends predicted by two other prior researchers.

CFD “virtual tracer studies” agreed well with experimental tracer studies and

mixing intensity predicted in CFD analyses of countercurrent flow also matched

dispersion estimates made in residence time distribution analyses. Peclet number

predicted in CFD analyses for the same range of gas flow rates as tracer studies agreed

very well with experimental data, especially for gas flow rates at and above 0.5 slpm.

CFD analyses also provided insights into the flow field and variation of mixing intensity

with height. In the vicinity of the sparger, large vortices are produced by the shear of the

down-flowing liquid by the up-flowing bubble plume. As gas flow rate is increased,

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these vortices elongate and the bubble plume changes from relatively straight and wide to

wavy and narrow as it rises in the column. The large vortices near the sparger back-mix

the liquid phase, making the region near the sparger well-mixed, despite poor distribution

of phases.

CFD showed the variation in mixing in the reactor to be non-uniform, with much

more intense mixing in the bottom of the reactor (near the sparger) than in the top of the

reactor. This distribution of mixing intensity would be changed significantly if inlet and

discharge configuration were different than those of the laboratory reactor. There are two

implications related to the importance of inlet and discharge configurations. First, in

addition to other scale-up laws, the influence of inlet and discharge configuration on pilot

column hydrodynamics must be considered when scaling to full scale. Second, if poor

hydraulic performance is realized in an ozone bubble contactor (e.g., T10 / is very low

or large fluctuations in ozone residuals occur at the reactor discharge), modifications to

inlets and discharges for chambers within the reactor offer relatively low-cost means of

improvement. Assessment of alternative modifications with a validated CFD model prior

to implementation could provide quantitative data on the effect of the alternatives faster,

cheaper and with more detail than experiments such as tracer studies or flow visualization

experiments.

A technique employing a reactive dye (indigo dye) and digital photography was

devised for allowing visualization of mass transfer and investigation of spatial variations

in mixing and mass transfer in the reactor. Inspection of images produced using this

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technique produced the following observations:

Indigo dye concentration and ozone dose can be selected to yield wide variation in

indigo dye concentration in the reactor.

In images of indigo dye flowing in the reactor, digital image pixel color varies

linearly with indigo dye concentration for indigo dye in the concentration range 0.5 to

6.5 mg/L.

Indigo dye decolors steadily and uniformly as water flows downward in the top of the

reactor.

Lower in the reactor, there are significant variations in indigo dye concentration at a

given reactor axial location.

Throughout the reactor, liquid flow occurs in two zones – upward flow in the bubble

plume and downward flow near the cylinder walls. Flow in the reactor is three

dimensional and unsteady, swirling and exhibiting chaotic motions. In the bottom of

the reactor, decoloration of indigo dye occurs as eddies of dye-rich water from the

downward flow are entrained into the bubble plume and decolored. Had aqueous

ozone not been immediately consumed by indigo dye, ozone concentration in the

bubble plume (and driving force for ozone mass transfer) would have been higher and

mass transfer in the vicinity of the bubbles would have been retarded.

Near the bottom of the reactor (near the sparger), there is a zone in which indigo dye

color is more or less uniform, indicating the liquid contents of that zone are well

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mixed. This zone is referred to as the entrance zone and its length increases with gas

to liquid flow ratio. As seen in CFD studies, this entrance zone is comprised of a

central upward flowing region (the bubble plume) driving large vortices between the

bubble plume and reactor walls.

To allow estimation of Peclet number, Stanton number and entrance zone length,

indigo concentration data from digital images were radially-averaged and the results were

fit using two models: a one-zone model in which the entire reactor was modeled using the

ADR model and a two-zone model in which the zone near the sparger was modeled as a

CSTR and in the upper zone the ADR model was used. Because data dependence could

not be disproved when the radially-averaged data were fit with the single zone model, it

was demonstrated that there are two distinct zones of different dispersion and perhaps

different mass transfer coefficient in the reactor. This finding is significant given the use

of single zone ADR or CSTR models for bubble column flows in pilot studies, full scale

reactor analyses and regulatory compliance.

Entrance region length increases with gas to liquid flow ratio. This finding is

consistent with CFD predictions that increasing gas flow rate stretches the large vortices

present in the vicinity of the sparger. At a gas to liquid flow ratio of 0.1, the entrance

region occupies nearly 40% of the reactor height. Future experiments should be directed

at determining the dependence of entrance length on water depth in the reactor. It is

hypothesized that entrance region length should be independent of water depth; since

momentum exchange between the bubble plume and downward flowing liquid

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establishes the vortices that define the entrance region, the entrance length should be

dependent on gas and liquid flow rates (momentum) and independent of water depth in

the reactor.

Stanton number increases with increasing gas to liquid flow ratio. Two

phenomena likely play roles in this trend. Higher gas flow rates result in both higher

specific surface area and increased turbulence and dispersion generated in bubbles’

wakes. In order to determine the roles these phenomena play in dependence of mass

transfer on gas to liquid flow ratio, the gas phase holdup must be measured. For the

reactor used in the current study, gas phase holdup at 5 points in the reactor could be

made using a differential pressure sensor. For a two dimensional reactor, gas phase

holdup could be estimated through analysis of digital photographs. Such an analysis

would involve bubble identification using particle identification techniques and summing

of bubble volumes within regions of the reactor.

Trends of Peclet number with gas to liquid flow ratio could not be determined

conclusively. All Peclet number estimates from indigo dye experiments followed trends

observed in RTD analyses except a single, low gas to liquid ratio datum at which Peclet

number was significantly less than expected. Indigo dye may have been completely

depleted in portions of the reactor in the experiment from which the anomalous Peclet

number was estimated.

As with mixing investigations, CFD analyses yielded details and insights into

countercurrent flow mass transfer. Most important, using an uncalibrated mass transfer

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model, the CFD model was able to accurately predict the variation in indigo dye

concentration in the reactor over the entire range of liquid and gas flow rates studied.

This agreement indicates that despite use of a two-equation turbulence model prone to

numerical dispersion, the CFD model predicted mixing of the main liquid flow with the

bubble plume sufficiently. Improvement in mass transfer and mixing predictions can be

expected if a higher-resolution turbulence model such as LES (large eddy simulation)

were used.

CFD simulations predicted and explained an increase in indigo concentration in

the vicinity of the sparger observed in numerous mass transfer visualization images.

Near the sparger, indigo dye rich water from the reactor walls is back-mixed into the

middle of the reactor, resulted in an apparent increase in indigo dye concentration.

VIII.3 Using CFD in Design and Scale-up of Ozone Bubble Contactors

Common use of the advection-dispersion-reaction (ADR) model (LeSauze et al.,

1993; Zhou and Smith 1994; El-Din and Smith 2001(a); Kim et al., 2002b; Kim et al.,

2005) and the CSTR model (US EPA Office of Drinking Water 1991; LeSauze et al.,

1993; Roustan et al., 1996; US EPA Office of Water 2003) for pilot and full scale ozone

bubble contactors implies that in countercurrent flow, phases are uniformly distributed

and contact between phases is uniform. The current study has shown that this is not the

case, even in the relatively simple tall cylindrical bubble column in which experiments

were performed. This discrepancy between models and hydrodynamics is significant –

modeling reactors as CSTRs provides a conservative estimate of inactivation in full scale

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ozone bubble contactors (Lev and Regli 1992a; Lev and Regli 1992b) but leads to

designs prone to unnecessary bromate production (Tang et al., 2005).

As an alternative to the ADR and CSTR models, CFD can deliver realistic

estimates for microbial inactivation and for chemical species whose rate of production

can be dependably represented by a set of elementary reactions or a global reaction

expression. These CFD models can be developed using mass transfer and bubble

transport submodels drawn from empirical and semi-empirical studies and using batch

kinetic data for chemical species and microorganisms. Unlike models such as the ADR

which are calibrated using data from pilot studies, CFD models are based on first-

principles submodels and have validity for reactors of virtually any geometry.

Application of CFD should no longer be limited to modeling and design of unit

process operations in very high production plants, as has been the tendency in the past.

The resources for producing the CFD models for this thesis (one student under the

direction of knowledgeable managers, a desktop computer and a software license) are

modest, making CFD accessible, either in-house or through subcontracts, to small utilities

in need of improved hydrodynamics, bromate production or design of new disinfection

unit operations.

Incorporation of CFD into pilot studies will allow improved scale-up to full scale.

As demonstrated in this study, RTD analyses, the most common technique used in pilot

reactor hydrodynamics characterization, is not suited to identifying important flowfield

features such as the well mixed zone in the reactor bottom, the large recirculating flows

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in the vicinity of the sparger, or the flow structures associated with inlets and outlets.

The inlet and outlet configuration may dominate pilot reactor hydrodynamics, as seen in

the Philadelphia Water Department pilot reactor. Given the importance of inlet and

discharge configuration, it would be advisable to perform CFD analysis as a part of the

pilot reactor design process.

Accurate depiction of hydrodynamics is important for accurate prediction of the

progress of chemical reactions in continuous flow reactors (Hermanowicz et al., 1999;

Tang et al., 2005). When chemical reactions are modeled as a sequence of elementary

reactions and the fate and transport of intermediate species is included in a CFD model,

CFD more accurately predicts the production/consumption of chemical species than

lower-fidelity models because chemical reactions occur based on the local concentration

of all species. There is a limit to the ability of CFD to incorporate species into a chemical

reaction model – each species adds to CPU time requirements of a solution and very

short-lived species or species whose reaction rate is very fast require very small time

steps to avoid numerical instability or overflows.

Finally, it is noted that most ozone bubble column reactors are similar in design.

Nearly all ozone contactors have over-under baffle arrangements and similar density of

spargers on the reactor floors. CFD could be used in a general exploration of the

influence of reactor geometry and operating conditions on hydraulic and disinfection

performance of reactors with different chamber aspect ratios, sparger spacings, baffle

configurations, gap widths, etc. A systematic study of these design parameters might

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yield guidelines for preliminary reactor designs and information helpful in scale-up from

cylindrical pilot reactors to full scale.

A specific design modification that should be investigated is exploration of the

impact of minor tilts in reactor walls on mixing in ozone contact chambers. As seen in

the current work and a prior study (Rice and Littlefield 1987), minor misalignment of a

tall cylindrical bubble column away from vertical can increase mixing by an order of

magnitude. A reactor designed to take advantage of this phenomenon would be a

significant improvement of existing reactors because vigorous mixing would promote

more even distribution of phases which, in turn, would result in greater mass transfer

rates and less propensity for the liquid phase to short circuit in ozone dissolution

chambers.

VIII.4 Critical Review of Ozone Mass Transfer Visualization Technique

The mass transfer visualization technique demonstrated in this study allowed

observation of spatial variation in mass transfer rate at a resolution heretofore unreported

in the literature and permitted estimation of a gas entrance length region.

Subsequent studies employing the mass transfer visualization technique can

benefit from several modifications.

Use of a two-dimensional reactor. The reactor used in this study was designed to be

comparable to pilot ozone bubble contactors used in prior studies and to promote, as

nearly as possible, axisymmetric flow. Though these goals were met in the reactor

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design, the curvature of the reactor distorted color near the reactor walls. Subsequent

studies might employ a tall, thin right rectangular cylindrical reactor. In such a

reactor, a rod sparger or different numbers and spacings of spherical spargers could

be employed. In addition to yielding better digital images, this design could be

modeled with a simpler CFD mesh (multi-block structured grid) and would allow

easier comparison of CFD results with images from mass transfer visualization

experiments.

Improved background lighting. An alternative lighting scheme that might provide

more intense, uniform lighting is shown in Figure 86. Optimization of this scheme

will require experimentation with the number and spacing of fluorescent tubes and the

thickness and material of the translucent plastic sheet.

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Translucent plastic sheet

High temperature fluorescent lamps

Reactor

Light baffles

Figure 86: Alternate Lighting Scheme

Performing all experiments at a single ozone generator voltage and indigo dye

concentration. The rationale for choosing the ozone voltage used in the experiments

in this study were achieving the greatest change in indigo dye color without

completely decoloring the dye within the reactor. Since the optimal voltage was not

known precisely for each experiment, multiple cases were run at different voltages for

some operating conditions. Influent indigo dye concentration also varied between

experiments. These variations in ozone dose and intake indigo dye concentration

made direct comparison of mass transfer (indigo consumption) from case to case

difficult. Based on the results of the indigo dye mass transfer visualization method

reported in this dissertation, future researchers should be able to select an adequate

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ozone generator voltage and indigo dye concentration for all experiments.

VIII.5 Balancing Acute and Chronic Risks

As outlined in section Chapter I, it is difficult to design reactors that afford a high

level of disinfection while not producing a harmful concentration of disinfection by-

products. Relatively long detention times provide a factor of safety and ensure

disinfection occurs to a desired level; relatively short residence times diminish

disinfection by-product formation. Balancing the acute microbial risks with chronic risks

from by-products may require more detailed understanding of the interaction of

hydrodynamics, chemistry and microbiology than has traditionally been established prior

to design of ozone bubble columns. Here, balancing means designing reactors with a

distribution of residence times that are long enough to ensure sufficient disinfection, but

not so long that excessive disinfection by-product formation occurs.

Hydrodynamics in bubble column reactors are complex and have a strong

influence on both microbial inactivation and disinfection byproduct formation. The

preceding work demonstrated that, because bubbled chambers tend to behave as CSTRs,

the US EPA’s approach of assigning Ct credit assuming CSTR behavior is justified and

does provide a conservative estimate of microbial inactivation. It also demonstrated that

in regard to bromate formation, producing reactors whose chambers behave as CSTRs is

not a conservative approach and is not protective of chronic risks from chemical

contaminants.

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The first step in balancing acute (microbial) and chronic (DBP) risks in fine

bubble ozone contactors is improved modeling and identification of hydrodynamics and

reactor designs that promote DBP formation. CFD is the only analysis available today

that incorporates all necessary processes with the level of detail needed to accurately

predict microbial inactivation and disinfection byproduct formation.

The second step is to design reactors with hydraulics in contact chambers closer

to plug flow. Developing such reactors will require experimentation. Tracer studies

have been used effectively in analysis of reactor hydraulics, but do not provide definitive

or specific information about the direction fluids flow in a given region in a reactor, so it

is recommended that experimentation be accompanied by CFD analyses. CFD modeling

can be less expensive than experimentation and could enable a wider range of design

alternatives.

Finally, current regulations and guidelines favor design of reactors that behave as

CSTRs. This approach is protective of acute risk but not chronic risk. Allowing use of

alternative models (beyond those permitted in the LT2ESWTR) for assessing disinfection

efficiency could encourage development of reactors designed to promote disinfection and

minimize DBP formation.

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APPENDIX A: LIST OF SYMBOLS

Variable Description

a Specific interfacial area

A Area

Bo Bond number

CD Drag coefficient

CI Indigo dye mass concentration

3OC Dissolved ozone mass concentration

dB Bubble diameter

Di Binary diffusion coefficient of species i

E Axial dispersion (L2/T)

E(t) Expectation

Eo Eotvos number

F Normalized tracer concentration

g Gravitational acceleration

Ga Galileo number

H Reactor height

IT Turbulent kinetic energy intensity

3BrOk Bromate reaction rate coefficient

kL Liquid side mass transfer coefficient

kN Microbial inactivation rate coefficient

3Ok Ozone autodecomposition reaction rate coefficient

m Henry’s law constant (dimensionless)

Mo Morton number

N Microorganism number density

NS Stanton number

P Pressure

Pe Peclet number

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272

Variable Description

TP Turbulent kinetic energy dissipation rate

Q Volumetric flow rate

Re Reynolds number

S Stripping factor

Sc Schmidt number

Sh Sherwood number

t Time

T10 Time for passage of 10% of pulse of conservative tracer

UG Gas superficial velocity

UL Liquid superficial velocity

U

Velocity

V Volume

vB Bubble terminal rise velocity

We Weber number

z Depth

z* Normalized depth

G Gas hold-up

Surface tension

Density

Kinematic viscosity

Dynamic viscosity

T Turbulent viscosity

G Gas volume fraction

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APPENDIX B: LIST OF ABBREVIATIONS AND ACRONYMS

Variable Description

ADR Advection-Dispersion-Reaction

CFD Computational Fluid Dynamics

CSTR Completely Stirred Tank Reactor

Ct Product of ozone residual concentration and time

DBP Disinfection Byproduct

HAA Haloacetic Acid

HDT Hydraulic Detention Time

LT2ESWTR` Long Term 2 Enhanced Surface Water Treatment Rule

NOM Natural Organic Matter

SWTR Surface Water Treatment Rule

TA Total Alkalinity

TOC Total Organic Carbon

USEPA United States Environmental ProtectionAgency

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APPENDIX C: ANALYSIS OF RADIALLY-AVERAGED IMAGE DATA

Radially-averaged indigo dye image data were used to estimate dispersion and

mass transfer rate in the column. The presence or absence of multiple zones was

determined via comparison of fit of single- and multiple-zone models to data.

Several models were formulated based on observed trends in indigo dye

consumption. At relatively high gas to liquid flow ratios, indigo dye concentration

reduced monotonically in the top of the reactor and was constant in the bottom of the

reactor. This observation prompted the formulation of the one-zone and two-zone

models described below. In the one-zone models, the mass transfer rate and dispersion

are assumed uniform in the reactor. In two-zone models, the bottom of the reactor is

assumed to behave as a continuously stirred tank reactor (CSTR) and it is assumed the

top of the reactor can be modeled as a 1-dimensional axial flow with dispersion and

reaction (1-D ADR) reactor. In one formulation of the two-zone model, the mass transfer

rate in the CSTR portion of the reactor is assumed to be different from that in the top half

of the reactor. In a second formulation, the mass transfer rate is assumed the same in the

top and bottom of the reactor and the difference in observed mass transfer in the two

regions is attributed wholly to difference in mixing.

Derivation of the single-zone and two-zone models follows.

Single-zone model

Conservation of gas phase ozone and aqueous indigo dye are depicted in Figure

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275

87. Gas phase dispersion (back-mixing of bubbles) is assumed to be negligible and

dissolved ozone is assumed to react very quickly with indigo dye.

dzACCak OOL aq*

g 33

zgOg CU *

3

dzzgOg CU

*

3

dz

z

dzACCak OOL aq*

g 33

zgOg CU *

3

dzzgOg CU

*

3

dz

zz

(a) Conservation of gas phase ozone (b) Conservation of aqueous indigo dye

dzA

dt

Cd

M

MR

gO

O

II

*

3

3

z

II

zIL

dz

dCD

CU

dz

dzz

II

dzzIL

dz

dCD

CU

z

dzA

dt

Cd

M

MR

gO

O

II

*

3

3

z

II

zIL

dz

dCD

CU

dz

dzz

II

dzzIL

dz

dCD

CU

zz

Figure 87: Conservation of Gas Phase Ozone and Aqueous Indigo Dye

Conservation of gas phase ozone

Conservation of mass about the control volume depicted in Figure 87(a) can be

written

dzCmCakCQCQ OGOLdzzGOGzGOG aq3333

where A is the column cross sectional area, QG is gas volumetric flow rate

(positive upward), kL is mass transfer coefficient (dimensions L/T), a is specific surface

Page 291: High resolution experimental studies and numerical ...

276

area (surface area per unit volume of reactor; dimensions L-1), GOC3

is gas phase ozone

mass concentration, aqOC3

is aqueous phase ozone mass concentration and m is the

Henry’s law constant (equilibrium gaseous ozone concentration equilibrium aqueous

ozone concentration). Henry’s law constant is calculated via the relation (Perry and

Chilton 1973) in equation 70 (repeated below)

C5C51687

2.6

C5C5840

25.3log

TT

TTm (70)

where T is temperature in degrees Kelvin and m is dimensionless.

Since the ozone-indigo dye reaction is very fast, aqueous ozone does not

accumulate and the conservation equation becomes

GO

G

LzGOdzzGOC

Um

ak

dz

CC

3

33

)(

)(

3

3

GO

G

LGO CUm

ak

dz

Cd (A-1)

Define Stanton number, stripping factor and dimensionless height as

;L

LS

U

HakN (A-2)

;L

G

U

UmS and (A-3)

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277

H

zz * . (A-4)

Equation A-1 becomes

*

)(

)(

3

3 dzS

N

C

CdS

GO

GO (A-5)

Equation A-5 is integrated from z* to the reactor bottom (z* = 1; gas injection

point). Denoting the gas injection ozone concentration as 03 GOC , the integration of

equation A-3 proceeds as follows:

*0

1

*

1ln

ln

3

3

*

03

33

zS

N

C

C

zS

NC

S

GO

GO

z

SC

CGO

GO

GO

*

33

1

0

zS

N

GOGO

S

eCC

and

*

33

1*

0*

zS

N

GOGO

S

eCC

(A-6)

where

m

CC

GO

GO3

3

* (A-7)

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278

Conservation of aqueous indigo dye

Conservation of indigo dye, depicted in Figure 87(b), can be written

dzARCQz

CDACQ

z

CDAdzA

t

CIdzzIL

dzz

I

zIL

z

II

where QL is liquid volumetric flow rate, CI is indigo trisulfonate concentration, D is

dispersion and RI is rate of indigo consumption. Assuming steady state conditions in the

column and that the ozone-indigo reaction is fast enough that rate of consumption of

indigo dye is equal to the mass transfer rate of ozone and noting that liquid superficial

velocity, UL, is equal to QL/A, the conservation of indigo dye can be written

dzCakM

M

dz

CCU

dz

dz

Cd

dz

Cd

D GOL

O

IzIdzzI

Lz

I

dzz

I

*

3

3

Substitute the expression from equation A-6 for *

3 GOC and, as dz 0, the

conservation of indigo dye becomes

*

3

3

1*

02

2 zS

N

GOL

O

IIL

I

S

eCakM

M

zd

CdU

zd

CdD

Introduce the dimensionless parameters z* = z / H and *IC =CI / CI 0, where CI 0 is indigo

dye concentration in the reactor feed. The nondimensionalized conservation of aqueous

indigo dye becomes

Page 294: High resolution experimental studies and numerical ...

279

*

3

3

1

0

*0

*

*

2*

*2z

S

N

LS

I

GO

O

IILIS

eD

HUS

S

N

C

C

M

M

zd

Cd

D

HU

zd

Cd

Define Peclet number and the parameter as

D

HUP L

e (A-8)

0,

0

0,

0 3

3

3

3 I

gO

L

G

O

I

I

gO

O

I

C

C

Q

Qm

M

MS

C

C

M

M (A-9)

Conservation of aqueous indigo dye becomes

*1

*

*

2*

*2 zS

N

eSI

eI

S

ePS

N

zd

CdP

zd

Cd

(A-10)

Equation A-10 is integrated as follows.

*1*

*

*

*

zS

N

eS

IeI

S

ePS

NCP

zd

Cd

zd

d

*1*

*

* zS

N

eIeI

S

ePCPzd

Cd(A-11)

where is an integration constant. Equation A-11 is solved using an integrating

factor:

Page 295: High resolution experimental studies and numerical ...

280

***

*

***

*

**

1*

1*

*

1*

*

zP

e

zS

NzP

eS

eI

zP

zS

N

ezP

IzP

zS

N

ei

zPdzP

e

Se

e

S

ee

S

ee

eP

ePSN

PCe

ePeCedz

d

ePpCpdz

d

eep

**1* zP

e

zSN

eS

eI

eS eP

ePSN

PC

(A-12)

and the rate of change of indigo dye concentration with respect to axial location is:

dCI*

dz*

NS S Pe

NS S Pe

e

NS S 1 z* Pe ePe z*

(A-13)

Determining integration constants for single zone model

Equation 11 is solved subject to a Dirichlet inlet boundary condition (CI = CI,0 at

z* = 0) and Danckwerts boundary condition at the outlet (dCI / dz*|z=1=0) (Nauman and

Buffham 1983; Teefy and Singer 1990; Haas et al., 1998). At the reactor discharge,

01

*

*

*

z

I

zd

Cd

ePe

eS

eS ePPSN

PSN

0

eP

eS

S ePSN

SN

Page 296: High resolution experimental studies and numerical ...

281

Substitute β into the expression for indigo dye concentration (equation A-11) and

simplify.

**1* zPP

eS

S

e

zSN

eS

eI

eeS eePSN

SN

Pe

PSN

PC

e

zPS

zSNe

eS

IP

eSNePPSN

C eS

** 11* (A-14)

A Dirichlet boundary condition is applied at the top of the reactor (z* = 0):

10

**

zIC (A-15)

e

PS

SNe

eS PeSNeP

PSNeS

1

eS P

SSN

e

eSe

eSNePPSNP

1

Substitute the expression for into equation 15 for the final expression for

aqueous indigo dye concentration.

eSe P

SSN

ezP

SzS

e

eS

I eSNePeSNePPSN

C

** 11* 1

**

111* zPPS

zSNSNe

eS

IeeSS eeSNeeP

PSNC

(A-16)

In the limit eS PSN , equation A-16 becomes indeterminate and an expression for

Page 297: High resolution experimental studies and numerical ...

282

dimensionless indigo dye concentration is determined using L’Hopital’s rule.

1

11lim

11lim

**

**

1* zPPzSNe

SNe

eS

eS

zPPS

zSNSNe

eS

eeSS

eeSS

eeePzeP

PSN

PSN

eeSNeeP

PSN

Substituting this result into equation A-16 yields the final expression for dimensionless

indigo dye concentration in the limit eS PSN :

e

PzPee

I PeezPPC

ee

ePS

SN

111*

lim

1*

*

(A-17)

Derivation of Governing Equations, Two Zone Model

The two-zone model, depicted in Figure 88, was developed based on observations

from ozone mass transfer visualization experiments that the near-sparger region (zone 2

[z* > zc*]) has a uniform indigo dye concentration whereas the in the top of the reactor

(zone 1 [z* < zc*]), indigo dye concentration increases monotonically with height. In the

two-zone model, zone 2 is modeled as well mixed (CSTR) and zone 1 is modeled using

the advection-dispersion-reaction model, as in the single-zone model described above.

The term zc* is the “critical” depth separating the two zones.

Page 298: High resolution experimental studies and numerical ...

283

*cz

1* z

Zone 1

Zone 2

1Zone2ZoneFlux2Zone1ZoneFlux

2zone;1zone; ****cIcI zzCzzC

Figure 88: Schematic Diagram, Two-Zone Model

Two-zone models were formulated assuming:

Equal Stanton number in zones 1 and 2

Different Stanton numbers in zones 1 and 2.

The derivation of these models is provided below.

Two Zone Model, Equal Stanton Numbers in Zones 1 and 2

Conservation of gaseous ozone in zone 2 is given as

cOLOGOG zHCakmCUmCU ***0 333

Page 299: High resolution experimental studies and numerical ...

284

HzCUm

aHkCC cO

G

LOO 1***

0 333

Recalling that Stanton number, stripping factor and dimensionless height are

given by

L

LS

U

aHkN

L

G

U

UmS

and

H

zz *

Gaseous ozone concentration in zone 2 becomes

*

*0*

113

3

cS

O

OzSN

CC

(A-18)

Conservation of gaseous ozone in zone 1 is determined by integrating equation A-2 from

z* to zc*

*

*

**3

**3

3

**lnccO

O

z

zS

zC

zCO zSNC

***

*

*0

3

3 ln11

ln zzSNCzS

CcSO

c

O

Page 300: High resolution experimental studies and numerical ...

285

**

3

3 *

*0*

11

zzSN

cS

O

OcSe

zSN

CC

(A-19)

Conservation of aqueous indigo dye in zone 2 is:

ACzHakM

MCQ

dz

dCDACQ OcL

O

IIL

zz

IIL

c

*2, 3

3**

Substitute for *

03OC from equation A-19 and nondimensionalize using 0,*

III CCC and

Hzz * .

*

*0*

2,*

*0,*

0,11

1 3

3** cS

O

cL

L

L

O

IIL

zz

II

IILzSN

CzU

U

aHk

M

MCU

dz

dC

H

CDCCU

c

*

*

*

*0

2,*

*

*

11

13

3** cS

c

I

OL

L

L

O

II

L

zz

ILI

zSN

z

C

C

D

HU

U

aHk

M

MC

D

HUC

D

HU

dz

dC

c

Recall that LLS UaHkN , LG UmUS and DHUP Le and define

0,

*0

0,

*0 3

3

3

3 I

O

O

I

I

O

L

G

O

I

C

CS

M

M

C

C

U

mU

M

M (A-20)

*

**

2,*

*

*

11

1

** cS

ceSIe

zz

IeI

zSN

zPSNCPCP

dz

dC

c

(A-21)

where

data

c

n

niiI

cdataI

I CnnC

C ,

0,

*2,

11(A-22)

Page 301: High resolution experimental studies and numerical ...

286

Conservation of aqueous indigo dye in zone 1 is given by

*

2

2

3

3

OL

O

IIL

I CakM

M

zd

CdU

zd

CdD

Nondimensionalize this expression and substitute for ozone concentration from

equation A-19:

**

3

3

*

*0

2

2

11zzSN

cS

O

L

O

IIL

I cSezSN

Cak

M

M

zd

CdU

zd

CdD

Rearranging this equation and introducing Stanton number, NS, Peclet number, Pe,

stripping factor, S, dimensionless height, z*, and dimensionless indigo dye concentration,

CI* yields the final expression for indigo dye concentration in zone 1.

**

*

*

2

*2

11

1 zzSN

cS

Se

Ie

I cSezSNS

NP

zd

CdP

zd

Cd

(A-23)

Equation A-23 is integrated as follows.

**

*

**

* 11

1 zzSN

cS

SeIe

I cSezSNS

NPCP

zd

dC

zd

d

**

*

**

11

1 zzSN

cS

eIeI cSe

zSNPCP

zd

dC(A-24)

The right hand side (RHS) of equation 20 is evaluated at z* = zc* and equated with the

RHS of equation 17 to determine an expression for the integration constant:

Page 302: High resolution experimental studies and numerical ...

287

eIe PCP *2,

Substitute the result into equation A-24.

**

*

*2,

**

11

1 zzSN

cS

eIeIeI cSe

zSNPCPCP

zd

dC

(A-25)

Equation A-25 is integrated using an integrating factor, yielding

****

*

*2,

*

* 11

1 zzSN

cS

eIezP

IzP cSee e

zSNPCPeCe

zd

d

***

*

*2,

*

11

1 zPzzSN

cSeS

eII

ecS eezSNPSN

PCC

(A-26)

where is an integration constant. The integration constant is determined using the inlet

boundary condition.

*

*

*2,

11

11 cS zSN

cSeS

eI e

zSNPSN

PC

Substitute the integration constant into equation 22 and rearrange for the final expression

for indigo dye concentration in zone 1.

****

**

*

*2,

*

11

1

1

cSecS

ee

zSNzPzzSN

cSeS

e

zPI

zPI

eezSNPSN

P

eCeC

(A-27)

Two Zone Model, Differing Stanton Numbers in Zones 1 and 2

In the two zone model in which Stanton number is allowed to differ in the zones,

Page 303: High resolution experimental studies and numerical ...

288

Stanton number in zones 1 and 2 are designated NS1 and NS2. Proceeding in a manner

similar to that used in the two-zone, single Stanton number model, gaseous ozone

concentration in zone 2 is given by

*2

*0*

113

3

cS

O

OzSN

CC

(A-28)

and concentration of gaseous ozone in zone 1 is given by

**

13

3 *2

*0*

11zzSN

cS

O

OcSe

zSN

CC

Conservation of aqueous indigo dye in zone 2 results in

*

2

*

2*

2,*

*

*

11

1

** cS

ceSIe

zz

IeI

zSN

zPSNCPCP

dz

dC

c

(A-29)

and the conservation of indigo dye in zone 1 is given by

**

1

*2

1*

2

*2

11

1 zzSN

cS

Se

Ie

I cSezSNS

NP

zd

CdP

zd

Cd

(A-30)

Equation A-30 is integrated twice and integration constants are determined using a

Dirichlet boundary condition at the inlet to zone 1 10

**

zIC and, at the discharge of

zone 1 (into zone 2) using the boundary condition

****

*

*

**

*

*

cc zz

IeI

zz

IeI CP

dz

dCCP

dz

dC

Page 304: High resolution experimental studies and numerical ...

289

The resulting expression for indigo dye concentration in zone 1 is

*

1***

1

**

*21

*2,

*

11

1

1

cSecS

ee

zSNzPzzSN

cSeS

e

zPI

zPI

eezSNPSN

P

eCeC

(A-31)

In the limit eS PSN , the expression for indigo dye concentration becomes

*2

**

2,*

111

**

**

cS

zzPezP

IzP

IzSN

ezPeCeC

ce

ee

(A-32)

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290

APPENDIX D: R SCRIPT FOR BEST FIT PARAMETERS ESTIMATION

cIndigo <- function(S1Hat, PeHat, S2Hat){exp(PeHat*Exp_Data2$zstar) +PeHat*psi*(exp(-S1Hat*(zc-Exp_Data2$zstar))-exp(-

S1Hat*zc+PeHat*Exp_Data2$zstar))/(S1Hat-PeHat)/(1+S2Hat*(1-zc)) +(CI2+psi)*(1-exp(PeHat*Exp_Data2$zstar))}

CIndigo <- function(p) {-sum((Exp_Data$MEAN - cIndigo(p[1],p[2]))^2)}

Exp_Data <- read.table("C:/Documents and Settings/Carolyn/MyDocuments/TBFiles/O3/IndigoPics/Finals/05_25_06/MEANS2_by16_Gurian.DAT",header=TRUE)

par(fig=c(0.025,0.975,0.025,0.975),mai=c(0.85,0.85,0.05,0.05))plot(Exp_Data$zstar,Exp_Data$MEAN,type="l",xlab=expression(z^a),ylab=expression(C[O[3]]^2),ylim=c(0,1))psi <- 1.1926

PeGuess <- 4S1Guess <- 1S2Guess <- 0

#### Plot model line using initial gueses##

ndata <- length(Exp_Data$zstar)nmin <- round(3*ndata/5)nmax <- ndata-1

nc <- nminzc <- Exp_Data$zstar[nc]

CI2 <- sum(Exp_Data$MEAN[nc:ndata])/(ndata - nc+1)SSE2 <- sum((Exp_Data$MEAN[nc:ndata]-CI2)^2)SSE2

MEAND <- Exp_Data$MEAN[1:nc]ZD <- Exp_Data$zstar[1:nc]Exp_Data2 <- data.frame(zstar=ZD, MEAN=MEAND)CI2min <- min(Exp_Data$MEAN)DCI2 <- MEAND[nc]-CI2minDCI2S2GuessX <- DCI2/(1-zc)/(psi-DCI2)S2Guess <- max(0,S2GuessX)S2GuessC <- cIndigo(S1Guess,PeGuess, S2Guess)lines(Exp_Data2$zstar,C,col="red")

Errs <- seq(length=ndata, from=-1e+6,by=0.000001)

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291

PeEstS <- seq(length=ndata, from=-1e+6,by=0.000001)S1EstS <- seq(length=ndata, from=-1e+6,by=0.000001)S2EstS <- seq(length=ndata, from=-1e+6,by=0.000001)

for (i in nmax:nmin) {nc <- izc <- Exp_Data$zstar[nc]ndata <- length(Exp_Data$zstar)

CI2 <- sum(Exp_Data$MEAN[nc:ndata])/(ndata - nc+1)SSE2 <- sum((Exp_Data$MEAN[nc:ndata]-CI2)^2)SSE2

MEAND <- Exp_Data$MEAN[1:nc]ZD <- Exp_Data$zstar[1:nc]Exp_Data2 <- data.frame(zstar=ZD, MEAN=MEAND)CI2min <- min(Exp_Data$MEAN)DCI2 <- MEAND[nc]-CI2minDCI2

genga <- nls.control(maxiter=10000,tol=1e-6,minFactor=0.000488281/128)outIndigo <- nls(MEAND ~ cIndigo(S1Est,PeEst, S2Est),Exp_Data2,start=

list(S1Est=S1Guess,PeEst=PeGuess,S2Est=S2Guess),genga,lower=c(0,0,0),algorithm="port")

AA <- coef(outIndigo)BB <- residuals(outIndigo)CC <- fitted.values(outIndigo)SSE1 <- sqrt(sum(BB^2))SSE1SSE2SSE <- SSE1 + SSE2SSE

S1Est <- AA[1]S1Guess <- S1EstPeEst <- AA[2]PeGuess <- PeEstS2Est <- AA[3]S2Guess <- S2EstiPeGuessS1GuessS2Guess

## CI <- cIndigo(S1Est,PeEst,S2Est)

lines(Exp_Data2$zstar,CC,col="blue")

zz <- Exp_Data$zstar[1:nc]CO31 <- exp(-S1Est*(zc-zz))/(1+S2Est*(1-zc))lines(zz,CO31,col="orange")

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292

z2line <- c(zc,1)CI2line <- c(CI2,CI2)CO32 <- 1/(1+S2Est*(1-zc))CO3Line <- c(CO32,CO32)lines(z2line,CI2line,col="blue")lines(z2line,CO3Line,col="orange")

Errs[i] <- SSES1EstS[i] <- S1EstS2EstS[i] <- S2EstPeEstS[i] <- PeEst}

ii <- seq(length=(nmax-nmin+1),from=nmin,by=1)imin <- which.min(abs(Errs))iminErrmin <- Errs[imin]ErrminErrmin <- min(abs(Errs))ErrminErrmax <- max(Errs)Errmaxplot(ii,Errs[nmin:nmax],xlab=expression(n[c]),ylab="SSE",ylim=c(Errmin,Errmax))points(imin,Errmin,col="red",cex=1.3,pch=19)

## Make a pretty plot showing fitted curves (indigo and ozone) and data

windows()par(fig=c(0.025,0.975,0.025,0.975),mai=c(0.85,0.85,0.05,0.05),family="serif",xaxs="r")gc <- grey(0:8 / 8)plot(Exp_Data$zstar,Exp_Data$MEAN,type="p",xlab="Normalized Depth(z*)",

ylab="Normalized Concentration",ylim=c(0,1),

xlim=c(0.2,1.0),col=gc[2],family="serif",cex.axis=1.25,cex.lab=1.25)

nc <- iminnczc <- Exp_Data$zstar[nc]zc

S1Guess <- S1EstS[imin]S1GuessS2Guess <- S2EstS[imin]S2GuessPeGuess <- PeEstS[imin]PeGuess

CI2 <- sum(Exp_Data$MEAN[nc:ndata])/(ndata - nc + 1)SSE2 <- sum((Exp_Data$MEAN[nc:ndata]-CI2)^2)

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293

SSE2

MEAND <- Exp_Data$MEAN[1:nc]ZD <- Exp_Data$zstar[1:nc]Exp_Data2 <- data.frame(zstar=ZD, MEAN=MEAND)genga <- nls.control(maxiter=100000,tol=1e-5)outIndigo <- nls(MEAND ~ cIndigo(S1Est,PeEst,S2Est),Exp_Data2,

start=list(S1Est=S1Guess,PeEst=PeGuess,S2Est=S2Guess),genga,lower=c(0,0,0),algorithm="port")

summary(outIndigo)iminExp_Data$zstar[imin]

AA <- coef(outIndigo)BB <- residuals(outIndigo)CC <- fitted.values(outIndigo)

S1Est <- AA[1]PeEst <- AA[2]S2Est <- AA[3]

SSE1 <- sqrt(sum(BB^2))SSE1SSE2SSE <- SSE1 + SSE2SSE

CI <- cIndigo(S1Est,PeEst,S2Est)

lines(Exp_Data2$zstar,CC,col="black",lwd=2)

zz <- Exp_Data$zstar[1:nc]CO31 <- exp(-S1Est*(zc-zz))/(1+S2Est*(1-zc))

z2line <- c(zc,1)CI2line <- c(CI2,CI2)CO32 <- 1/(1+S2Est*(1-zc))CO3Line <- c(CO32,CO32)lines(z2line,CI2line,col="black",lwd=2)legend(0.5,0.3,legend=c(expression(C[I]^"\*"*"\ "*"(Experimentaldata)"),expression(C[I]^"\*"*"\ "*"(Fitted model)")),col=c(gc[2],gc[0]),lty=c(0,1),lwd=c(1,2),bty="n",pch=c(1,26),y.intersp=1.3,cex=1.25,pt.cex=0.75)

#### Perform runs test on the residuals. Convert residuals to binaryarray and## factor, then perform the runs test##

ResBi <- sign(BB)

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294

ErrB <- seq(length=nc, from=-1e+6,by=0.000001)for (i in 1:nc) {ErrB[i] <- max(0,ResBi[i]) }ErrBF <- factor(ErrB)runs.test(ErrBF,alternative="two.sided")

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295

Vita

Timothy Allen Bartrand was born in Muskegon, Michigan, USA, on Octboer 19th,

1961 to Loren L. Bartrand and Donna Hickey Bartrand. Mr. Bartrand attended Rogers

High School, Wyoming, MI, graduating the class valedictorian. Upon graduation from

high school Mr. Bartrand undertook undergraduate studies at the University of Notre

Dame, Notre Dame, IN, earning a bachelor’s degree in aerospace engineering in May,

1983. In June, 1983, Mr. Bartrand began service as a Peace Corps volunteer, teaching

mathematics and physics at the Union Comprehensive Secondary School in Bachuo

Akagbe, Manyu Division, Southwest Province, Cameroon. He is married to Carolyn

Davis and they have one daughter, Olivia Davis Bartrand.

Mr. Bartrand has earned two masters degrees: a master of science in mechanical

engineering from the University of Tennessee (awarded 12/87, thesis title “A Study of

Low-Frequency Combustion Instability in Rocket Engine Preburners using a

Heterogeneous Stirred Tank Reactor Model”) and a master of science in civil engineering

from Ohio University (awarded 12/97, thesis title “Experimental Investigation of a

Vacuum Apparatus for Zebra Mussel Control in Closed Conduits”).

Mr. Bartrand’s professional experience includes eight years as a research engineer

working as a NASA Lewis Research Center on-site contractor, three years experience

developing water and sanitation facilities in relief settings and one year as an

environmental regulator for the Ohio EPA.

Page 311: High resolution experimental studies and numerical ...

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